Changes between Version 14 and Version 15 of GravoTurbulence


Ignore:
Timestamp:
07/01/11 15:02:14 (14 years ago)
Author:
Jonathan
Comment:

Legend:

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Added
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  • GravoTurbulence

    v14 v15  
    170170[[CollapsibleEnd]]
    171171[[CollapsibleStart(Alphabetically)]]
    172 
    173  [http://adsabs.harvard.edu/abs/2002 Sci...295...93A Abel et al 2002] The Formation of the First Star in the Universe
    174 * [http://adsabs.harvard.edu/abs/2001 ApJ...552..639A Aikawa et al 2001] Molecular Evolution in Collapsing Prestellar Cores
    175 * [http://adsabs.harvard.edu/abs/2003 ApJ...593..906A Aikawa et al 2003] Molecular Evolution in Collapsing Prestellar Cores. II. The Effect of Grain-Surface Reactions
    176 * [http://adsabs.harvard.edu/abs/2005 ApJ...620..330A Aikawa et al 2005]Molecular Evolution in Collapsing Prestellar Cores. III. Contraction of a Bonnor-Ebert Sphere
    177 * [http://adsabs.harvard.edu/abs/1999 ApJ...515..286B Ballesteros-Paredes 1999] Clouds as Turbulent Density Fluctuations: Implications for Pressure Confinement and Spectral Line Data Interpretation
    178 * [http://adsabs.harvard.edu/abs/1999 ApJ...527..285B Ballesteros-Paredes 1999] Turbulent Flow-driven Molecular Cloud Formation: A Solution to the Post-T Tauri Problem
    179 * [http://adsabs.harvard.edu/abs/2003 ApJ...592..188B Ballesteros-Paredes 2003] Dynamic cores in hydrostatic disguise
    180  * SPH Turbulent driving of various sorts with self-gravity turned on. (Periodic BC) 205379 particles
    181 * [http://adsabs.harvard.edu/abs/2006 ApJ...637..384B Ballesteros-Paredes 2006] The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function
    182 * [http://adsabs.harvard.edu/abs/2006 MNRAS.372..443B Ballesteros-Paredes 2006] Six myths on the virial theorem for interstellar clouds
    183 * [http://adsabs.harvard.edu/abs/2007 prpl.conf...63B Ballesteros-Paredes 2007] Molecular Cloud Turbulence and Star Formation
    184 * [http://adsabs.harvard.edu/abs/2011 MNRAS.411...65B Ballesteros-Paredes 2011] Gravity or turbulence? Velocity dispersion-size relation
    185 * [http://adsabs.harvard.edu/abs/2011 arXiv1105.5411B Ballesteros-Paredes 2011] Gravity or turbulence? II. Evolving column density PDFs in molecular clouds
    186 * [http://adsabs.harvard.edu/abs/2009 MNRAS.398.1082B Banerjee et al 2009] Clump morphology and evolution in MHD simulations of molecular cloud formation
    187 * [http://adsabs.harvard.edu/abs/1998 ApJ...508L..95B Bate 1998] Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations
    188 * [http://adsabs.harvard.edu/abs/1987 A%26A...172..293B Bonazzola et al, 1987] Jeans collapse in a turbulent medium
    189 * [http://adsabs.harvard.edu/abs/2006 MNRAS.370..488B Bonnell and Bate 2006] Star formation through gravitational collapse and competitive accretion
    190 * [http://adsabs.harvard.edu/abs/2006 MNRAS.368.1296B Bonnell and Bate 2006] The Jeans mass and the origin of the knee in the IMF
    191 * [http://adsabs.harvard.edu/abs/1980 ApJ...236..619B Boss 1980] Protostellar formation in rotating interstellar clouds. I -0 Numerical methods and tests
    192 * [http://adsabs.harvard.edu/abs/1980 ApJ...237..563B Boss 1980] Protostellar formation in rotating interstellar clouds. II -0 Axially symmetric collapse
    193 * [http://adsabs.harvard.edu/abs/1980 ApJ...237..866B Boss 1980] Protostellar formation in rotating interstellar clouds. III -0 Nonaxisymmetric collapse
    194 * [http://adsabs.harvard.edu/abs/1984 ApJ...277..768B Boss 1984] Protostellar formation in rotating interstellar clouds. IV Nonisothermal collapse
    195 * [http://adsabs.harvard.edu/abs/1986 ApJS...62..519B Boss 1986] Protostellar formation in rotating interstellar clouds. V -0 Nonisothermal collapse and fragmentation
    196 * [http://adsabs.harvard.edu/abs/1987 ApJ...319..149B Boss 1987] Protostellar formation in rotating interstellar clouds. VI -0 Nonuniform initial conditions
    197 * [http://adsabs.harvard.edu/abs/1988 ApJ...331..370B Boss 1988] Protostellar formation in rotating interstellar clouds. VII -0 Opacity and fragmentation
    198 * [http://adsabs.harvard.edu/abs/1989 ApJ...346..336B Boss 1989] Protostellar formation in rotating interstellar clouds. VIII -0 Inner core formation
    199 * [http://adsabs.harvard.edu/abs/1993 ApJ...410..157B Boss 1993] Collapse and fragmentation of molecular cloud cores. I -0 Moderately centrally condensed cores
    200 * [http://adsabs.harvard.edu/abs/1995 ApJ...439..224B Boss 1995] Collapse and fragmentation of molecular cloud cores. 2: Collapse induced by stellar shock waves
    201 * [http://adsabs.harvard.edu/abs/1995 ApJ...451..218B Boss 1995] Collapse and Fragmentation of Molecular Cloud Cores. III. Initial Differential Rotation
    202 * [http://adsabs.harvard.edu/abs/1996 ApJ...468..231B Boss 1996] Collapse and Fragmentation of Molecular Cloud Cores. IV. Oblate Clouds and Small Cluster Formation
    203 * [http://adsabs.harvard.edu/abs/1997 ApJ...483..309B Boss 1997] Collapse and Fragmentation of Molecular Cloud Cores. V. Loss of Magnetic Field Support
    204 * [http://adsabs.harvard.edu/abs/1999 ApJ...520..744B Boss 1999] Collapse and Fragmentation of Molecular Cloud Cores. VI. Slowly Rotating Magnetic Clouds
    205 * [http://adsabs.harvard.edu/abs/2000 ApJ...528..325B Boss et al 2000] The Jeans Condition and Collapsing Molecular Cloud Cores: Filaments or Binaries
    206 * [http://adsabs.harvard.edu/abs/2001 ApJ...562..842B Boss & Hartmann 2001] Protostellar Collapse in a Rotating, Self-gravitating Sheet
    207 * [http://adsabs.harvard.edu/abs/2002 ApJ...568..743B Boss 2002] Collapse and Fragmentation of Molecular Cloud Cores. VII. Magnetic Fields and Multiple Protostar Formation
    208 * [http://adsabs.harvard.edu/abs/2005 ApJ...622..393B Boss 2005] Collapse and Fragmentation of Molecular Cloud Cores. VIII. Magnetically Supported Infinite Sheets
    209 * [http://adsabs.harvard.edu/abs/2007 astro.ph..1210B Boss 2007] Collapse and Fragmentation of Molecular Cloud Cores. IX. Magnetic Braking of Initially Filamentary Clouds
    210 * [http://adsabs.harvard.edu/abs/2011 MNRAS.410L...8C Cho & Kim 2011] Enhanced core formation rate in a turbulent cloud by self-gravity
     172* [http://adsabs.harvard.edu/abs/2002Sci...295...93A Abel et al 2002] The Formation of the First Star in the Universe
     173* [http://adsabs.harvard.edu/abs/2001ApJ...552..639A Aikawa et al 2001] Molecular Evolution in Collapsing Prestellar Cores
     174* [http://adsabs.harvard.edu/abs/2003ApJ...593..906A Aikawa et al 2003] Molecular Evolution in Collapsing Prestellar Cores. II. The Effect of Grain-Surface Reactions
     175* [http://adsabs.harvard.edu/abs/2005ApJ...620..330A Aikawa et al 2005]Molecular Evolution in Collapsing Prestellar Cores. III. Contraction of a Bonnor-Ebert Sphere
     176* [http://adsabs.harvard.edu/abs/1999ApJ...515..286B Ballesteros-Paredes 1999] Clouds as Turbulent Density Fluctuations: Implications for Pressure Confinement and Spectral Line Data Interpretation
     177* [http://adsabs.harvard.edu/abs/1999ApJ...527..285B Ballesteros-Paredes 1999] Turbulent Flow-driven Molecular Cloud Formation: A Solution to the Post-T Tauri Problem
     178* [http://adsabs.harvard.edu/abs/2003ApJ...592..188B Ballesteros-Paredes 2003] Dynamic cores in hydrostatic disguise
     179 * SPH Turbulent driving of various sorts with self-gavity turned on. (Periodic BC) 205379 particles
     180* [http://adsabs.harvard.edu/abs/2006ApJ...637..384B Ballesteros-Paredes 2006] The Mass Spectra of Cores in Turbulent Molecular Clouds and Implications for the Initial Mass Function
     181* [http://adsabs.harvard.edu/abs/2006MNRAS.372..443B Ballesteros-Paredes 2006] Six myths on the virial theorem for interstellar clouds
     182* [http://adsabs.harvard.edu/abs/2007prpl.conf...63B Ballesteros-Paredes 2007] Molecular Cloud Turbulence and Star Formation
     183* [http://adsabs.harvard.edu/abs/2011MNRAS.411...65B Ballesteros-Paredes 2011] Gravity or turbulence? Velocity dispersion-size relation
     184* [http://adsabs.harvard.edu/abs/2011arXiv1105.5411B Ballesteros-Paredes 2011] Gravity or turbulence? II. Evolving column density PDFs in molecular clouds
     185* [http://adsabs.harvard.edu/abs/2009MNRAS.398.1082B Banerjee et al 2009] Clump morphology and evolution in MHD simulations of molecular cloud formation
     186* [http://adsabs.harvard.edu/abs/1998ApJ...508L..95B Bate 1998] Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations
     187* [http://adsabs.harvard.edu/abs/1987A%26A...172..293B Bonazzola et al, 1987] Jeans collapse in a turbulent medium
     188* [http://adsabs.harvard.edu/abs/2006MNRAS.370..488B Bonnell and Bate 2006] Star formation through gravitational collapse and competitive accretion
     189* [http://adsabs.harvard.edu/abs/2006MNRAS.368.1296B Bonnell and Bate 2006] The Jeans mass and the origin of the knee in the IMF
     190* [http://adsabs.harvard.edu/abs/1980ApJ...236..619B Boss 1980] Protostellar formation in rotating interstellar clouds. I -0 Numerical methods and tests
     191* [http://adsabs.harvard.edu/abs/1980ApJ...237..563B Boss 1980] Protostellar formation in rotating interstellar clouds. II -0 Axially symmetric collapse
     192* [http://adsabs.harvard.edu/abs/1980ApJ...237..866B Boss 1980] Protostellar formation in rotating interstellar clouds. III -0 Nonaxisymmetric collapse
     193* [http://adsabs.harvard.edu/abs/1984ApJ...277..768B Boss 1984] Protostellar formation in rotating interstellar clouds. IV Nonisothermal collapse
     194* [http://adsabs.harvard.edu/abs/1986ApJS...62..519B Boss 1986] Protostellar formation in rotating interstellar clouds. V -0 Nonisothermal collapse and fragmentation
     195* [http://adsabs.harvard.edu/abs/1987ApJ...319..149B Boss 1987] Protostellar formation in rotating interstellar clouds. VI -0 Nonuniform initial conditions
     196* [http://adsabs.harvard.edu/abs/1988ApJ...331..370B Boss 1988] Protostellar formation in rotating interstellar clouds. VII -0 Opacity and fragmentation
     197* [http://adsabs.harvard.edu/abs/1989ApJ...346..336B Boss 1989] Protostellar formation in rotating interstellar clouds. VIII -0 Inner core formation
     198* [http://adsabs.harvard.edu/abs/1993ApJ...410..157B Boss 1993] Collapse and fragmentation of molecular cloud cores. I -0 Moderately centrally condensed cores
     199* [http://adsabs.harvard.edu/abs/1995ApJ...439..224B Boss 1995] Collapse and fragmentation of molecular cloud cores. 2: Collapse induced by stellar shock waves
     200* [http://adsabs.harvard.edu/abs/1995ApJ...451..218B Boss 1995] Collapse and Fragmentation of Molecular Cloud Cores. III. Initial Differential Rotation
     201* [http://adsabs.harvard.edu/abs/1996ApJ...468..231B Boss 1996] Collapse and Fragmentation of Molecular Cloud Cores. IV. Oblate Clouds and Small Cluster Formation
     202* [http://adsabs.harvard.edu/abs/1997ApJ...483..309B Boss 1997] Collapse and Fragmentation of Molecular Cloud Cores. V. Loss of Magnetic Field Support
     203* [http://adsabs.harvard.edu/abs/1999ApJ...520..744B Boss 1999] Collapse and Fragmentation of Molecular Cloud Cores. VI. Slowly Rotating Magnetic Clouds
     204* [http://adsabs.harvard.edu/abs/2000ApJ...528..325B Boss et al 2000] The Jeans Condition and Collapsing Molecular Cloud Cores: Filaments or Binaries
     205* [http://adsabs.harvard.edu/abs/2001ApJ...562..842B Boss & Hartmann 2001] Protostellar Collapse in a Rotating, Self-gravitating Sheet
     206* [http://adsabs.harvard.edu/abs/2002ApJ...568..743B Boss 2002] Collapse and Fragmentation of Molecular Cloud Cores. VII. Magnetic Fields and Multiple Protostar Formation
     207* [http://adsabs.harvard.edu/abs/2005ApJ...622..393B Boss 2005] Collapse and Fragmentation of Molecular Cloud Cores. VIII. Magnetically Supported Infinite Sheets
     208* [http://adsabs.harvard.edu/abs/2007astro.ph..1210B Boss 2007] Collapse and Fragmentation of Molecular Cloud Cores. IX. Magnetic Braking of Initially Filamentary Clouds
     209* [http://adsabs.harvard.edu/abs/2011MNRAS.410L...8C Cho & Kim 2011] Enhanced core formation rate in a turbulent cloud by self-gravity
    211210 * 512^3^ Isothermal MHD fixed grid
    212211 * beta=.1
     
    215214 * Power law tail
    216215 * Line-width size relation
    217 * [http://adsabs.harvard.edu/abs/2010 MNRAS.409L..39C Ciardi & Hennebelle 2010] Outflows and mass accretion in collapsing dense cores with misaligned rotation axis and magnetic field
    218 * [http://adsabs.harvard.edu/abs/2005 MNRAS.361....2C Clark and Bonnell 2005] The onset of collapse in turbulently supported molecular clouds
    219 * [http://adsabs.harvard.edu/abs/2011 ApJ...727..110C Clark et al 2011] Gravitational Fragmentation in Turbulent Primordial Gas and the Initial Mass Function of Population III Stars
    220 * [http://adsabs.harvard.edu/abs/1980 ApJ...242..765C Cohn 1980] Late core collapse in star clusters and the gravothermal instability
    221 * [http://adsabs.harvard.edu/abs/2011 ApJ...731...59C Collins et al 2011] Mass and Magnetic Distributions in Self-gravitating Super-Alfvénic Turbulence with Adaptive Mesh Refinement
     216* [http://adsabs.harvard.edu/abs/2010MNRAS.409L..39C Ciardi & Hennebelle 2010] Outflows and mass accretion in collapsing dense cores with misaligned rotation axis and magnetic field
     217* [http://adsabs.harvard.edu/abs/2005MNRAS.361....2C Clark and Bonnell 2005] The onset of collapse in turbulently supported molecular clouds
     218* [http://adsabs.harvard.edu/abs/2011ApJ...727..110C Clark et al 2011] Gravitational Fragmentation in Turbulent Primordial Gas and the Initial Mass Function of Population III Stars
     219* [http://adsabs.harvard.edu/abs/1980ApJ...242..765C Cohn 1980] Late core collapse in star clusters and the gravothermal instability
     220* [http://adsabs.harvard.edu/abs/2011ApJ...731...59C Collins et al 2011] Mass and Magnetic Distributions in Self-gravitating Super-Alfvénic Turbulence with Adaptive Mesh Refinement
    222221 * ENZO 128^3^+4 = 2048^3^; 10pc -> 1000 AU; MHD Isothermal 10K; n=300/cc; B=.6+-2.7 microG (no AD) (supercritical)
    223222 * power law tail for density (1.64) and B (2.74)
     
    225224 * sigma = rho^.25^ for cores
    226225 * CMF = 2.1+-.6
    227 * [http://adsabs.harvard.edu/abs/2002 NuPhB.625..409D de Vega & Sanchez 2002] Statistical mechanics of the self-gravitating gas: I. Thermodynamic limit and phase diagrams
    228 * [http://adsabs.harvard.edu/abs/2002 ApJ...577..206E Elmegreen 2002] Star Formation from Galaxies to Globules
    229 * [http://adsabs.harvard.edu/abs/1992 A%26A...257..715F Falgarone 1992] The small-scale density and velocity structure of quiescent molecular clouds
    230 * [http://adsabs.harvard.edu/abs/2010 ApJ...713..269F Federrath et al 2010] Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH
    231 * [http://adsabs.harvard.edu/abs/2010 A%26A...512A..81F Federrath et al 2010] Comparing the statistics of interstellar turbulence in simulations and observations. Solenoidal versus compressive turbulence forcing
    232 * [http://adsabs.harvard.edu/abs/1992 ApJ...391..199F Fiedler & Mouschovias 1992] Ambipolar diffusion and star formation: Formation and contraction of axisymmetric cloud cores. I -0 Formulation of the problem and method of solution
    233 * [http://adsabs.harvard.edu/abs/1993 ApJ...415..680F Fiedler & Mouschovias 1993] Ambipolar Diffusion and Star Formation: Formation and Contraction of Axisymmetric Cloud Cores. II. Results
    234 * [http://adsabs.harvard.edu/abs/1984 ApJ...281....1F Fillmore & Goldreich 1984] Self-similar gravitational collapse in an expanding universe
    235 * [http://adsabs.harvard.edu/abs/1993 ApJ...416..303F Foster & Chevalier 1993] Gravitational Collapse of an Isothermal Sphere
    236 * [http://adsabs.harvard.edu/abs/2008 ApJ...676.1109F Furesz et al. 2008] Kinematic Structure of the Orion Nebula Cluster and its Surroundings
    237 * [http://adsabs.harvard.edu/abs/1993 ApJ...417..220G Galli & Shu 1993] Collapse of Magnetized Molecular Cloud Cores. I. Semianalytical Solution
    238 * [http://adsabs.harvard.edu/abs/1993 ApJ...417..243G Galli & Shu 1993] Collapse of Magnetized Molecular Cloud Cores. II. Numerical Results
    239 * [http://adsabs.harvard.edu/abs/1996 ApJ...462..725G Gammie 1996] Linear Theory of Magnetized, Viscous, Self-gravitating Gas Disks
    240 * [http://adsabs.harvard.edu/abs/1996 ApJ...466..814G Gammie & Ostriker 1996] Can Nonlinear Hydromagnetic Waves Support a Self-gravitating Cloud
    241 * [http://adsabs.harvard.edu/abs/2007 ApJS..169..239G Glover & Mac Low 2007] Simulating the Formation of Molecular Clouds. I. Slow Formation by Gravitational Collapse from Static Initial Conditions
    242 * [http://adsabs.harvard.edu/abs/2007 ApJ...659.1317G Glover & Mac Low 2007] Simulating the Formation of Molecular Clouds. II. Rapid Formation from Turbulent Initial Conditions* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009Natur.457...63G&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Goodman et al. 2009
    243 * [http://adsabs.harvard.edu/abs/1980 ApJ...238..991G Goldreich & Weber 1980] Homologously collapsing stellar cores
    244 * [http://adsabs.harvard.edu/abs/2004 A%26A...414..633G Goodwin et al. 2004] Simulating star formation in molecular cloud cores. I. The influence of low levels of turbulence on fragmentation and multiplicity
    245 * [http://adsabs.harvard.edu/abs/2004 A%26A...423..169G Goodwin et al. 2004] Simulating star formation in molecular cores. II. The effects of different levels of turbulence
    246 * [http://adsabs.harvard.edu/abs/1994 ApJ...430L..49H Hartmann et al 1994] Protostellar collapse in a self-gravitating sheet
    247 * [http://adsabs.harvard.edu/abs/1996 ApJ...464..387H Hartmann et al 1996] Sheet Models of Protostellar Collapse
    248 * [http://adsabs.harvard.edu/abs/2001 ApJ...562..852H Hartmann et al. 2001] Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
    249 * [http://adsabs.harvard.edu/abs/2000 ApJ...535..887K Heitsch et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
    250 * [http://adsabs.harvard.edu/abs/2001 ApJ...547..280H Heitsch et al 2001] Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
    251 * [http://adsabs.harvard.edu/abs/2005 ApJ...633L.113H Heitsch et al 2005] Formation of Structure in Molecular Clouds: A Case Study
    252 * [http://adsabs.harvard.edu/abs/2006 ApJ...648.1052H Heitsch et al 2006] The Birth of Molecular Clouds: Formation of Atomic Precursors in Colliding Flows
    253 * [http://adsabs.harvard.edu/abs/2008 ApJ...674..316H Heitsch et al 2008] Cooling, Gravity, and Geometry: Flow-driven Massive Core Formation
    254 * [http://adsabs.harvard.edu/abs/2008 ApJ...689..290H Heitsch & Hartmann 2008] Rapid Molecular Cloud and Star Formation: Mechanisms and Movies
    255 * [http://adsabs.harvard.edu/abs/2000 A%26A...359.1124H Hennebelle & Perault 2000] Dynamical condensation in a magnetized and thermally bistable flow. Application to interstellar cirrus
    256 * [http://adsabs.harvard.edu/abs/2003 MNRAS.340..870H Hennebelle et al. 2003] Protostellar collapse induced by compression
    257 * [http://adsabs.harvard.edu/abs/2004 MNRAS.348..687H Hennebelle et al. 2004] Protostellar collapse induced by compression -0 II. Rotation and fragmentation
    258 * [http://adsabs.harvard.edu/abs/2007 arXiv0711.2417H Hennebelle et al 2007] Diffuse interstellar medium and the formation of molecular clouds
    259 * [http://adsabs.harvard.edu/abs/2008 A%26A...486L..43H Hennebelle et al. 2008] From the warm magnetized atomic medium to molecular clouds
    260 * [http://adsabs.harvard.edu/abs/2008 ApJ...684..395H Hennebelle & Chabrier 2008] Analytical Theory for the Initial Mass Function: CO Clumps and Prestellar Cores
    261 * [http://adsabs.harvard.edu/abs/2009 ApJ...702.1428H Hennebelle & Chabrier 2009] Analytical Theory for the Initial Mass Function. II. Properties of the Flow
    262 * [http://adsabs.harvard.edu/abs/2009 ApJ...699.1092H Heyer et al. 2009] Re-Examining Larson's Scaling Relationships in Galactic Molecular Clouds
    263 * [http://adsabs.harvard.edu/abs/2011 arXiv1101.4940H Hopkins et al 2011] Self-Regulated Star Formation in Galaxies via Momentum Input from Massive Stars
    264 * [http://adsabs.harvard.edu/abs/1962 ApJ...136..594H Hunter 1962] The Instability of the Collapse of a Self-Gravitating Gas Cloud
    265 * [http://adsabs.harvard.edu/abs/1977 ApJ...218..834H Hunter 1977] The collapse of unstable isothermal spheres
    266 * [http://adsabs.harvard.edu/abs/1986 ApJ...305..309H Hunter et al 1986] Star formation in colliding gas flows
    267 * [http://adsabs.harvard.edu/abs/2005 A%26A...435..611J Jappsen et al 2005] The stellar mass spectrum from non-isothermal gravoturbulent fragmentation
    268 * [http://adsabs.harvard.edu/abs/1998 ApJ...501L.205K Klessen et al 1998] Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster
    269 * [http://adsabs.harvard.edu/abs/2000 ApJS..128..287K Klessen et al 2000] The Formation of Stellar Clusters: Gaussian Cloud Conditions. I.x
    270 * [http://adsabs.harvard.edu/abs/2000 ApJ...535..887K Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
    271 * [http://adsabs.harvard.edu/abs/2000 ApJ...535..869K Klessen et al 2000] One-Point Probability Distribution Functions of Supersonic Turbulent Flows in Self-gravitating Media
    272 * [http://adsabs.harvard.edu/abs/2001 ApJ...547..280H Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
    273 * [http://adsabs.harvard.edu/abs/2001 ApJ...556..837K Klessen 2001] The Formation of Stellar Clusters: Mass Spectra from Turbulent Molecular Cloud Fragmentation
    274 * [http://adsabs.harvard.edu/abs/2005 ApJ...620..786K Klessen et al 2005] Quiescent and Coherent Cores from Gravoturbulent Fragmentation
    275 * [http://adsabs.harvard.edu/abs/2011 ApJ...727L..20K Kritsuk et al 2011] On the Density Distribution in Star-forming Interstellar Clouds
     226* [http://adsabs.harvard.edu/abs/2002NuPhB.625..409D de Vega & Sanchez 2002] Statistical mechanics of the self-gravitating gas: I. Thermodynamic limit and phase diagrams
     227* [http://adsabs.harvard.edu/abs/2002ApJ...577..206E Elmegreen 2002] Star Formation from Galaxies to Globules
     228* [http://adsabs.harvard.edu/abs/1992A%26A...257..715F Falgarone 1992] The small-scale density and velocity structure of quiescent molecular clouds
     229* [http://adsabs.harvard.edu/abs/2010ApJ...713..269F Federrath et al 2010] Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH
     230* [http://adsabs.harvard.edu/abs/2010A%26A...512A..81F Federrath et al 2010] Comparing the statistics of interstellar turbulence in simulations and observations. Solenoidal versus compressive turbulence forcing
     231* [http://adsabs.harvard.edu/abs/1992ApJ...391..199F Fiedler & Mouschovias 1992] Ambipolar diffusion and star formation: Formation and contraction of axisymmetric cloud cores. I -0 Formulation of the problem and method of solution
     232* [http://adsabs.harvard.edu/abs/1993ApJ...415..680F Fiedler & Mouschovias 1993] Ambipolar Diffusion and Star Formation: Formation and Contraction of Axisymmetric Cloud Cores. II. Results
     233* [http://adsabs.harvard.edu/abs/1984ApJ...281....1F Fillmore & Goldreich 1984] Self-similar gravitational collapse in an expanding universe
     234* [http://adsabs.harvard.edu/abs/1993ApJ...416..303F Foster & Chevalier 1993] Gravitational Collapse of an Isothermal Sphere
     235* [http://adsabs.harvard.edu/abs/2008ApJ...676.1109F Furesz et al. 2008] Kinematic Structure of the Orion Nebula Cluster and its Surroundings
     236* [http://adsabs.harvard.edu/abs/1993ApJ...417..220G Galli & Shu 1993] Collapse of Magnetized Molecular Cloud Cores. I. Semianalytical Solution
     237* [http://adsabs.harvard.edu/abs/1993ApJ...417..243G Galli & Shu 1993] Collapse of Magnetized Molecular Cloud Cores. II. Numerical Results
     238* [http://adsabs.harvard.edu/abs/1996ApJ...462..725G Gammie 1996] Linear Theory of Magnetized, Viscous, Self-gravitating Gas Disks
     239* [http://adsabs.harvard.edu/abs/1996ApJ...466..814G Gammie & Ostriker 1996] Can Nonlinear Hydromagnetic Waves Support a Self-gravitating Cloud
     240* [http://adsabs.harvard.edu/abs/2007ApJS..169..239G Glover & Mac Low 2007] Simulating the Formation of Molecular Clouds. I. Slow Formation by Gravitational Collapse from Static Initial Conditions
     241* [http://adsabs.harvard.edu/abs/2007ApJ...659.1317G Glover & Mac Low 2007] Simulating the Formation of Molecular Clouds. II. Rapid Formation from Turbulent Initial Conditions* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009Natur.457...63G&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Goodman et al. 2009
     242* [http://adsabs.harvard.edu/abs/1980ApJ...238..991G Goldreich & Weber 1980] Homologously collapsing stellar cores
     243* [http://adsabs.harvard.edu/abs/2004A%26A...414..633G Goodwin et al. 2004] Simulating star formation in molecular cloud cores. I. The influence of low levels of turbulence on fragmentation and multiplicity
     244* [http://adsabs.harvard.edu/abs/2004A%26A...423..169G Goodwin et al. 2004] Simulating star formation in molecular cores. II. The effects of different levels of turbulence
     245* [http://adsabs.harvard.edu/abs/1994ApJ...430L..49H Hartmann et al 1994] Protostellar collapse in a self-gravitating sheet
     246* [http://adsabs.harvard.edu/abs/1996ApJ...464..387H Hartmann et al 1996] Sheet Models of Protostellar Collapse
     247* [http://adsabs.harvard.edu/abs/2001ApJ...562..852H Hartmann et al. 2001] Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
     248* [http://adsabs.harvard.edu/abs/2000ApJ...535..887K Heitsch et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
     249* [http://adsabs.harvard.edu/abs/2001ApJ...547..280H Heitsch et al 2001] Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
     250* [http://adsabs.harvard.edu/abs/2005ApJ...633L.113H Heitsch et al 2005] Formation of Structure in Molecular Clouds: A Case Study
     251* [http://adsabs.harvard.edu/abs/2006ApJ...648.1052H Heitsch et al 2006] The Birth of Molecular Clouds: Formation of Atomic Precursors in Colliding Flows
     252* [http://adsabs.harvard.edu/abs/2008ApJ...674..316H Heitsch et al 2008] Cooling, Gravity, and Geometry: Flow-driven Massive Core Formation
     253* [http://adsabs.harvard.edu/abs/2008ApJ...689..290H Heitsch & Hartmann 2008] Rapid Molecular Cloud and Star Formation: Mechanisms and Movies
     254* [http://adsabs.harvard.edu/abs/2000A%26A...359.1124H Hennebelle & Perault 2000] Dynamical condensation in a magnetized and thermally bistable flow. Application to interstellar cirrus
     255* [http://adsabs.harvard.edu/abs/2003MNRAS.340..870H Hennebelle et al. 2003] Protostellar collapse induced by compression
     256* [http://adsabs.harvard.edu/abs/2004MNRAS.348..687H Hennebelle et al. 2004] Protostellar collapse induced by compression -0 II. Rotation and fragmentation
     257* [http://adsabs.harvard.edu/abs/2007arXiv0711.2417H Hennebelle et al 2007] Diffuse interstellar medium and the formation of molecular clouds
     258* [http://adsabs.harvard.edu/abs/2008A%26A...486L..43H Hennebelle et al. 2008] From the warm magnetized atomic medium to molecular clouds
     259* [http://adsabs.harvard.edu/abs/2008ApJ...684..395H Hennebelle & Chabrier 2008] Analytical Theory for the Initial Mass Function: CO Clumps and Prestellar Cores
     260* [http://adsabs.harvard.edu/abs/2009ApJ...702.1428H Hennebelle & Chabrier 2009] Analytical Theory for the Initial Mass Function. II. Properties of the Flow
     261* [http://adsabs.harvard.edu/abs/2009ApJ...699.1092H Heyer et al. 2009] Re-Examining Larson's Scaling Relationships in Galactic Molecular Clouds
     262* [http://adsabs.harvard.edu/abs/2011arXiv1101.4940H Hopkins et al 2011] Self-Regulated Star Formation in Galaxies via Momentum Input from Massive Stars
     263* [http://adsabs.harvard.edu/abs/1962ApJ...136..594H Hunter 1962] The Instability of the Collapse of a Self-Gravitating Gas Cloud
     264* [http://adsabs.harvard.edu/abs/1977ApJ...218..834H Hunter 1977] The collapse of unstable isothermal spheres
     265* [http://adsabs.harvard.edu/abs/1986ApJ...305..309H Hunter et al 1986] Star formation in colliding gas flows
     266* [http://adsabs.harvard.edu/abs/2005A%26A...435..611J Jappsen et al 2005] The stellar mass spectrum from non-isothermal gravoturbulent fragmentation
     267* [http://adsabs.harvard.edu/abs/1998ApJ...501L.205K Klessen et al 1998] Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster
     268* [http://adsabs.harvard.edu/abs/2000ApJS..128..287K Klessen et al 2000] The Formation of Stellar Clusters: Gaussian Cloud Conditions. I.x
     269* [http://adsabs.harvard.edu/abs/2000ApJ...535..887K Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
     270* [http://adsabs.harvard.edu/abs/2000ApJ...535..869K Klessen et al 2000] One-Point Probability Distribution Functions of Supersonic Turbulent Flows in Self-gravitating Media
     271* [http://adsabs.harvard.edu/abs/2001ApJ...547..280H Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
     272* [http://adsabs.harvard.edu/abs/2001ApJ...556..837K Klessen 2001] The Formation of Stellar Clusters: Mass Spectra from Turbulent Molecular Cloud Fragmentation
     273* [http://adsabs.harvard.edu/abs/2005ApJ...620..786K Klessen et al 2005] Quiescent and Coherent Cores from Gravoturbulent Fragmentation
     274* [http://adsabs.harvard.edu/abs/2011ApJ...727L..20K Kritsuk et al 2011] On the Density Distribution in Star-forming Interstellar Clouds
    276275 * ENZO 512^3^+5x2=524,288^3^; 5pc -> 2 AU; Isothermal 10K; n=500/cc
    277276 * Power law tail to density pdf
    278 * [http://adsabs.harvard.edu/abs/2007 ApJ...656..959K Krumholz et al 2007] Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores
    279 * [http://adsabs.harvard.edu/abs/2011 ApJ...731...25K Krumholz et al 2011] Which Phase of the Interstellar Medium Correlates with the Star Formation Rate
    280 * [http://adsabs.harvard.edu/abs/1981 MNRAS.194..809L Larson 1981] Turbulence and star formation in molecular clouds
    281 * [http://adsabs.harvard.edu/abs/1985 MNRAS.214..379L Larson 1985] Cloud fragmentation and stellar masses
    282 * [http://adsabs.harvard.edu/abs/2003 RPPh...66.1651L Larson 2003] The physics of star formation
    283 * [http://adsabs.harvard.edu/abs/2000 AAS...197.0502L Li et al 2000] Simulations of Star Formation out of a Turbulence Molecular Cloud
    284 * [http://adsabs.harvard.edu/abs/2003 ApJ...592..975L Li et al 2003] The Formation of Stellar Clusters in Turbulent Molecular Clouds: Effects of the Equation of State
    285 * [http://adsabs.harvard.edu/abs/2005 ApJ...618..344V Li et al 2004] The Lifetimes and Evolution of Molecular Cloud Cores
    286 * [http://adsabs.harvard.edu/abs/2005 ApJ...620L..19L Li et al 2005] Control of Star Formation in Galaxies by Gravitational Instability
    287 * [http://adsabs.harvard.edu/abs/1965 ApJ...142.1431L Lin et al 1965] The Gravitational Collapse of a Uniform Spheroid
    288 * [http://adsabs.harvard.edu/abs/1976 MNRAS.176..367L Low & Lyndin-Bell] The minimum Jeans mass or when fragmentation must stop
    289 * [http://adsabs.harvard.edu/abs/1998 ApJ...495..346M Masunaga et al. 1998] A Radiation Hydrodynamic Model for Protostellar Collapse. I. The First Collapse
    290 * [http://adsabs.harvard.edu/abs/2000 ApJ...531..350M Masunaga & Inutsuka 2000] A Radiation Hydrodynamic Model for Protostellar Collapse. II. The Second Collapse and the Birth of a Protostar
    291 * [http://adsabs.harvard.edu/abs/2007 ARA%26A..45..565M McKee Ostriker 2007] Theory of Star Formation
    292 * [http://adsabs.harvard.edu/abs/1997 ApJ...476..750M McLaughlin & Pudritz 1997] Gravitational Collapse and Star Formation in Logotropic and Nonisothermal Spheres
    293 * [http://adsabs.harvard.edu/abs/1984 ApJ...279..621M Miyama et al 1984] Criteria for collapse and fragmentation of rotating, isothermal clouds
    294 * [http://adsabs.harvard.edu/abs/1976 ApJ...206..753M Mouschovias 1976] Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: Star formation. I Formulation of the problem and method of solution
    295 * [http://adsabs.harvard.edu/abs/1976 ApJ...207..141M Mouschovias 1976] Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: Star formation. II -0 Results
    296 * [http://adsabs.harvard.edu/abs/1976 ApJ...210..326M Mouschovias & Spitzer 1976] Note on the collapse of magnetic interstellar clouds
    297 * [http://adsabs.harvard.edu/abs/1991 ApJ...373..169M Mouschovias 1991] Magnetic braking, ambipolar diffusion, cloud cores, and star formation -0 Natural length scales and protostellar masses
    298 * [http://adsabs.harvard.edu/abs/2008 ApJ...687..354N Nakamura & Li 2008] Magnetically Regulated Star Formation in Three Dimensions: The Case of the Taurus Molecular Cloud Complex
     277* [http://adsabs.harvard.edu/abs/2007ApJ...656..959K Krumholz et al 2007] Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores
     278* [http://adsabs.harvard.edu/abs/2011ApJ...731...25K Krumholz et al 2011] Which Phase of the Interstellar Medium Correlates with the Star Formation Rate
     279* [http://adsabs.harvard.edu/abs/1981MNRAS.194..809L Larson 1981] Turbulence and star formation in molecular clouds
     280* [http://adsabs.harvard.edu/abs/1985MNRAS.214..379L Larson 1985] Cloud fragmentation and stellar masses
     281* [http://adsabs.harvard.edu/abs/2003RPPh...66.1651L Larson 2003] The physics of star formation
     282* [http://adsabs.harvard.edu/abs/2000AAS...197.0502L Li et al 2000] Simulations of Star Formation out of a Turbulence Molecular Cloud
     283* [http://adsabs.harvard.edu/abs/2003ApJ...592..975L Li et al 2003] The Formation of Stellar Clusters in Turbulent Molecular Clouds: Effects of the Equation of State
     284* [http://adsabs.harvard.edu/abs/2005ApJ...618..344V Li et al 2004] The Lifetimes and Evolution of Molecular Cloud Cores
     285* [http://adsabs.harvard.edu/abs/2005ApJ...620L..19L Li et al 2005] Control of Star Formation in Galaxies by Gravitational Instability
     286* [http://adsabs.harvard.edu/abs/1965ApJ...142.1431L Lin et al 1965] The Gravitational Collapse of a Uniform Spheroid
     287* [http://adsabs.harvard.edu/abs/1976MNRAS.176..367L Low & Lyndin-Bell] The minimum Jeans mass or when fragmentation must stop
     288* [http://adsabs.harvard.edu/abs/1998ApJ...495..346M Masunaga et al. 1998] A Radiation Hydrodynamic Model for Protostellar Collapse. I. The First Collapse
     289* [http://adsabs.harvard.edu/abs/2000ApJ...531..350M Masunaga & Inutsuka 2000] A Radiation Hydrodynamic Model for Protostellar Collapse. II. The Second Collapse and the Birth of a Protostar
     290* [http://adsabs.harvard.edu/abs/2007ARA%26A..45..565M McKee Ostriker 2007] Theory of Star Formation
     291* [http://adsabs.harvard.edu/abs/1997ApJ...476..750M McLaughlin & Pudritz 1997] Gravitational Collapse and Star Formation in Logotropic and Nonisothermal Spheres
     292* [http://adsabs.harvard.edu/abs/1984ApJ...279..621M Miyama et al 1984] Criteria for collapse and fragmentation of rotating, isothermal clouds
     293* [http://adsabs.harvard.edu/abs/1976ApJ...206..753M Mouschovias 1976] Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: Star formation. I Formulation of the problem and method of solution
     294* [http://adsabs.harvard.edu/abs/1976ApJ...207..141M Mouschovias 1976] Nonhomologous contraction and equilibria of self-gravitating, magnetic interstellar clouds embedded in an intercloud medium: Star formation. II -0 Results
     295* [http://adsabs.harvard.edu/abs/1976ApJ...210..326M Mouschovias & Spitzer 1976] Note on the collapse of magnetic interstellar clouds
     296* [http://adsabs.harvard.edu/abs/1991ApJ...373..169M Mouschovias 1991] Magnetic braking, ambipolar diffusion, cloud cores, and star formation -0 Natural length scales and protostellar masses
     297* [http://adsabs.harvard.edu/abs/2008ApJ...687..354N Nakamura & Li 2008] Magnetically Regulated Star Formation in Three Dimensions: The Case of the Taurus Molecular Cloud Complex
    299298 * 128^3^ isothermal MHD with AD and feedback 2.4 pc -> 0.02 pc
    300299 * B=15 microG (beta=1/24) subcritical
    301 * [http://adsabs.harvard.edu/abs/1998 ApJ...494..587N Nakano 1998] Star Formation in Magnetic Clouds
    302 * [http://adsabs.harvard.edu/abs/2008 ApJ...686.1174O Offner et al 2008] Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
     300* [http://adsabs.harvard.edu/abs/1998ApJ...494..587N Nakano 1998] Star Formation in Magnetic Clouds
     301* [http://adsabs.harvard.edu/abs/2008ApJ...686.1174O Offner et al 2008] Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
    303302 * 1100/cc 10K
    304 * [http://adsabs.harvard.edu/abs/2008 AJ....136..404O Offner et al. 2008] The Kinematics of Molecular Cloud Cores in the Presence of Driven and Decaying Turbulence: Comparisons with Observations
    305 * [http://adsabs.harvard.edu/abs/2009 ApJ...693..914O Offner et al 2009] The Shapes of Molecular Cloud Cores in Simulations and Observations
    306 * [http://adsabs.harvard.edu/abs/2001 A%26A...379.1005O Ossenkopf 2001] On the structure of self-gravitating molecular clouds
    307 * [http://adsabs.harvard.edu/abs/1999 ApJ...513..259O Ostriker 1999] Kinetic and Structural Evolution of Self-gravitating, Magnetized Clouds: 2.5-dimensional Simulations of Decaying Turbulence
    308 * [http://adsabs.harvard.edu/abs/2001 ApJ...546..980O Ostriker 2001] Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models
    309 * [http://adsabs.harvard.edu/abs/2002 ApJ...576..870P Padoan & Nordlund 2002] The Stellar Initial Mass Function from Turbulent Fragmentation
    310 * [http://adsabs.harvard.edu/abs/2011 ApJ...730...40P Padoan & Nordlund 2011] The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence
    311 * [http://adsabs.harvard.edu/abs/1969 MNRAS.145..457P Penston 1969] Dynamics of self-gravitating gaseous spheres-II. Collapses of gas spheres with cooling and the behaviour of polytropic gas spheres
    312 * [http://adsabs.harvard.edu/abs/1969 MNRAS.144..425P Penston 1969] Dynamics of self-gravitating gaseous spheres-III. Analytical results in the free-fall of isothermal cases
    313 * [http://adsabs.harvard.edu/abs/2011 ApJ...729...72P Peters et al 2011] The Interplay of Magnetic Fields, Fragmentation, and Ionization Feedback in High-mass Star Formation
    314 * [http://adsabs.harvard.edu/abs/2007 MNRAS.377...77P Price & Bate 2007] The impact of magnetic fields on single and binary star formation
    315 * [http://adsabs.harvard.edu/abs/2008 MNRAS.385.1820P Price & Bate 2008] The effect of magnetic fields on star cluster formation
    316 * [http://adsabs.harvard.edu/abs/2009 MNRAS.398...33P Price & Bate 2009] Inefficient star formation: the combined effects of magnetic fields and radiative feedback
    317 * [http://adsabs.harvard.edu/abs/1997 ASPC..123..117P Pudritz et al 1997] Collapse and Outflow: Towards an Integrated Theory of Star Formation
    318 * [http://adsabs.harvard.edu/abs/1977 MNRAS.179..541R Rees & Ostriker 1977] Cooling, dynamics and fragmentation of massive gas clouds -0 Clues to the masses and radii of galaxies and clusters
    319 * [http://adsabs.harvard.edu/abs/1977 ApJ...214..488S Shu 1977] Self-similar collapse of isothermal spheres and star formation
    320 * [http://adsabs.harvard.edu/abs/1989 ApJ...342..834L Shu & Lizano 1989] Molecular cloud cores and bimodal star formation
    321 * [http://adsabs.harvard.edu/abs/1987 ARA%26A..25...23S Shu, Adams, & Lizano 1987] Star formation in molecular clouds -0 Observation and theory
    322 * [http://adsabs.harvard.edu/abs/1977 ApJ...214..152S Silk 1977] On the fragmentation of cosmic gas clouds. II -0 Opacity-limited star formation
    323 * [http://adsabs.harvard.edu/abs/1966 MNRAS.132..359S Strittmatter 1966] Gravitational collapse in the presence of a magnetic field
    324 * [http://adsabs.harvard.edu/abs/1984 ApJ...286..529T Tereby, Shu, & Cassen 1984] The collapse of the cores of slowly rotating isothermal clouds
    325 * [http://adsabs.harvard.edu/abs/2010 ApJ...714L..58T Tomida 2010] Radiation Magnetohydrodynamics Simulation of Proto-stellar Collapse: Two-component Molecular Outflow
    326 * [http://adsabs.harvard.edu/abs/1997 ApJ...489L.179T Truelove 1997] The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-gravitational Hydrodynamics
    327 * [http://adsabs.harvard.edu/abs/1998 ApJ...495..821T Truelove et al. 1998] Self-gravitational Hydrodynamics with Three-dimensional Adaptive Mesh Refinement: Methodology and Applications to Molecular Cloud Collapse and Fragmentation
    328 * [http://adsabs.harvard.edu/abs/2003 ApJ...585L.131V Vazques-Semadeni et al 2003] A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency: First Tests
    329 * [http://adsabs.harvard.edu/abs/2003 ASPC..287...81V Vazques-Semadeni et al. 2003] The Origin of Molecular Cloud Turbulence and its Role on Determining the Star Formation Efficiency
    330 * [http://adsabs.harvard.edu/abs/2006 ApJ...643..245V Vazques-Semadeni et al 2006] Molecular Cloud Evolution. I. Molecular Cloud and Thin Cold Neutral Medium Sheet Formation
    331 * [http://adsabs.harvard.edu/abs/2007 ApJ...657..870V Vazques-Semadeni et al 2007] Molecular Cloud Evolution. II. From Cloud Formation to the Early Stages of Star Formation in Decaying Conditions
    332 * [http://adsabs.harvard.edu/abs/2005 ApJ...618..344V Vazquez-Semadeni 2005] The Lifetimes and Evolution of Molecular Cloud Cores
    333 * [http://adsabs.harvard.edu/abs/2005 ApJ...630L..49V Vazquez-Semadeni et al. 2005] Star Formation Efficiency in Driven, Supercritical, Turbulent Clouds
    334 * [http://adsabs.harvard.edu/abs/2010 ApJ...709...27W Wang et al 2010] Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster-Forming Clumps
    335 * [http://adsabs.harvard.edu/abs/1976 ApJ...207..484W Woodward 1976] Shock-driven implosion of interstellar gas clouds and star formation
    336 
     303* [http://adsabs.harvard.edu/abs/2008AJ....136..404O Offner et al. 2008] The Kinematics of Molecular Cloud Cores in the Presence of Driven and Decaying Turbulence: Comparisons with Observations
     304* [http://adsabs.harvard.edu/abs/2009ApJ...693..914O Offner et al 2009] The Shapes of Molecular Cloud Cores in Simulations and Observations
     305* [http://adsabs.harvard.edu/abs/2001A%26A...379.1005O Ossenkopf 2001] On the structure of self-gravitating molecular clouds
     306* [http://adsabs.harvard.edu/abs/1999ApJ...513..259O Ostriker 1999] Kinetic and Structural Evolution of Self-gravitating, Magnetized Clouds: 2.5-dimensional Simulations of Decaying Turbulence
     307* [http://adsabs.harvard.edu/abs/2001ApJ...546..980O Ostriker 2001] Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models
     308* [http://adsabs.harvard.edu/abs/2002ApJ...576..870P Padoan & Nordlund 2002] The Stellar Initial Mass Function from Turbulent Fragmentation
     309* [http://adsabs.harvard.edu/abs/2011ApJ...730...40P Padoan & Nordlund 2011] The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence
     310* [http://adsabs.harvard.edu/abs/1969MNRAS.145..457P Penston 1969] Dynamics of self-gravitating gaseous spheres-II. Collapses of gas spheres with cooling and the behaviour of polytropic gas spheres
     311* [http://adsabs.harvard.edu/abs/1969MNRAS.144..425P Penston 1969] Dynamics of self-gravitating gaseous spheres-III. Analytical results in the free-fall of isothermal cases
     312* [http://adsabs.harvard.edu/abs/2011ApJ...729...72P Peters et al 2011] The Interplay of Magnetic Fields, Fragmentation, and Ionization Feedback in High-mass Star Formation
     313* [http://adsabs.harvard.edu/abs/2007MNRAS.377...77P Price & Bate 2007] The impact of magnetic fields on single and binary star formation
     314* [http://adsabs.harvard.edu/abs/2008MNRAS.385.1820P Price & Bate 2008] The effect of magnetic fields on star cluster formation
     315* [http://adsabs.harvard.edu/abs/2009MNRAS.398...33P Price & Bate 2009] Inefficient star formation: the combined effects of magnetic fields and radiative feedback
     316* [http://adsabs.harvard.edu/abs/1997ASPC..123..117P Pudritz et al 1997] Collapse and Outflow: Towards an Integrated Theory of Star Formation
     317* [http://adsabs.harvard.edu/abs/1977MNRAS.179..541R Rees & Ostriker 1977] Cooling, dynamics and fragmentation of massive gas clouds -0 Clues to the masses and radii of galaxies and clusters
     318* [http://adsabs.harvard.edu/abs/1977ApJ...214..488S Shu 1977] Self-similar collapse of isothermal spheres and star formation
     319* [http://adsabs.harvard.edu/abs/1989ApJ...342..834L Shu & Lizano 1989] Molecular cloud cores and bimodal star formation
     320* [http://adsabs.harvard.edu/abs/1987ARA%26A..25...23S Shu, Adams, & Lizano 1987] Star formation in molecular clouds -0 Observation and theory
     321* [http://adsabs.harvard.edu/abs/1977ApJ...214..152S Silk 1977] On the fragmentation of cosmic gas clouds. II -0 Opacity-limited star formation
     322* [http://adsabs.harvard.edu/abs/1966MNRAS.132..359S Strittmatter 1966] Gravitational collapse in the presence of a magnetic field
     323* [http://adsabs.harvard.edu/abs/1984ApJ...286..529T Tereby, Shu, & Cassen 1984] The collapse of the cores of slowly rotating isothermal clouds
     324* [http://adsabs.harvard.edu/abs/2010ApJ...714L..58T Tomida 2010] Radiation Magnetohydrodynamics Simulation of Proto-stellar Collapse: Two-component Molecular Outflow
     325* [http://adsabs.harvard.edu/abs/1997ApJ...489L.179T Truelove 1997] The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-gravitational Hydrodynamics
     326* [http://adsabs.harvard.edu/abs/1998ApJ...495..821T Truelove et al. 1998] Self-gravitational Hydrodynamics with Three-dimensional Adaptive Mesh Refinement: Methodology and Applications to Molecular Cloud Collapse and Fragmentation
     327* [http://adsabs.harvard.edu/abs/2003ApJ...585L.131V Vazques-Semadeni et al 2003] A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency: First Tests
     328* [http://adsabs.harvard.edu/abs/2003ASPC..287...81V Vazques-Semadeni et al. 2003] The Origin of Molecular Cloud Turbulence and its Role on Determining the Star Formation Efficiency
     329* [http://adsabs.harvard.edu/abs/2006ApJ...643..245V Vazques-Semadeni et al 2006] Molecular Cloud Evolution. I. Molecular Cloud and Thin Cold Neutral Medium Sheet Formation
     330* [http://adsabs.harvard.edu/abs/2007ApJ...657..870V Vazques-Semadeni et al 2007] Molecular Cloud Evolution. II. From Cloud Formation to the Early Stages of Star Formation in Decaying Conditions
     331* [http://adsabs.harvard.edu/abs/2005ApJ...618..344V Vazquez-Semadeni 2005] The Lifetimes and Evolution of Molecular Cloud Cores
     332* [http://adsabs.harvard.edu/abs/2005ApJ...630L..49V Vazquez-Semadeni et al. 2005] Star Formation Efficiency in Driven, Supercritical, Turbulent Clouds
     333* [http://adsabs.harvard.edu/abs/2010ApJ...709...27W Wang et al 2010] Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster-Forming Clumps
     334* [http://adsabs.harvard.edu/abs/1976ApJ...207..484W Woodward 1976] Shock-driven implosion of interstellar gas clouds and star formation
    337335[[CollapsibleEnd]]