Changes between Version 13 and Version 14 of GravoTurbulence


Ignore:
Timestamp:
07/01/11 14:59:04 (14 years ago)
Author:
Jonathan
Comment:

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  • GravoTurbulence

    v13 v14  
    22
    33== References ==
    4 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002Sci...295...93A&db_key=AST&link_type=ABSTRAhttp://adsabs.harvard.edu/abs/2002Sci...295...93A Abel et al 2002] The Formation of the First Star in the Universe
    5 * [http://adsabs.harvard.edu/abs/2001ApJ...552..639A Aikawa et al 2001] Molecular Evolution in Collapsing Prestellar Cores
    6 * [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
    7 * [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
    8 * [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
    9 * [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?
    10 * [http://adsabs.harvard.edu/abs/2003ApJ...592..188B Ballesteros-Paredes 2003] Dynamic cores in hydrostatic disguise
    11  * SPH Turbulent driving of various sorts with self-gravity turned on. (Periodic BC) 205,379 particles
    12 * [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
    13 * [http://adsabs.harvard.edu/abs/2006MNRAS.372..443B Ballesteros-Paredes 2006] Six myths on the virial theorem for interstellar clouds
    14 * [http://adsabs.harvard.edu/abs/2007prpl.conf...63B Ballesteros-Paredes 2007] Molecular Cloud Turbulence and Star Formation
    15 * [http://adsabs.harvard.edu/abs/2011MNRAS.411...65B Ballesteros-Paredes 2011] Gravity or turbulence? Velocity dispersion-size relation
    16 * [http://adsabs.harvard.edu/abs/2011arXiv1105.5411B Ballesteros-Paredes 2011] Gravity or turbulence? II. Evolving column density PDFs in molecular clouds
    17 * [http://adsabs.harvard.edu/abs/2009MNRAS.398.1082B Banerjee et al 2009] Clump morphology and evolution in MHD simulations of molecular cloud formation
    18 * [http://adsabs.harvard.edu/abs/1998ApJ...508L..95B Bate 1998] Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations
    19 * [http://adsabs.harvard.edu/abs/1987A%26A...172..293B Bonazzola et al, 1987] Jeans collapse in a turbulent medium
    20 * [http://adsabs.harvard.edu/abs/2006MNRAS.370..488B Bonnell and Bate 2006] Star formation through gravitational collapse and competitive accretion
    21 * [http://adsabs.harvard.edu/abs/2006MNRAS.368.1296B Bonnell and Bate 2006] The Jeans mass and the origin of the knee in the IMF
     4[[CollapsibleStart(Chronologically)]]
     5
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    2422* [http://adsabs.harvard.edu/abs/1980ApJ...237..866B Boss 1980] Protostellar formation in rotating interstellar clouds. III - Nonaxisymmetric collapse
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     28* [http://adsabs.harvard.edu/abs/1984ApJ...279..621M Miyama et al 1984] Criteria for collapse and fragmentation of rotating, isothermal clouds
     29* [http://adsabs.harvard.edu/abs/1984ApJ...286..529T Tereby, Shu, & Cassen 1984] The collapse of the cores of slowly rotating isothermal clouds
     30* [http://adsabs.harvard.edu/abs/1985MNRAS.214..379L Larson 1985] Cloud fragmentation and stellar masses
    2631* [http://adsabs.harvard.edu/abs/1986ApJS...62..519B Boss 1986] Protostellar formation in rotating interstellar clouds. V - Nonisothermal collapse and fragmentation
     32* [http://adsabs.harvard.edu/abs/1986ApJ...305..309H Hunter et al 1986] Star formation in colliding gas flows
     33* [http://adsabs.harvard.edu/abs/1987A%26A...172..293B Bonazzola et al, 1987] Jeans collapse in a turbulent medium
    2734* [http://adsabs.harvard.edu/abs/1987ApJ...319..149B Boss 1987] Protostellar formation in rotating interstellar clouds. VI - Nonuniform initial conditions
     35* [http://adsabs.harvard.edu/abs/1987ARA%26A..25...23S Shu, Adams, & Lizano 1987] Star formation in molecular clouds - Observation and theory
    2836* [http://adsabs.harvard.edu/abs/1988ApJ...331..370B Boss 1988] Protostellar formation in rotating interstellar clouds. VII - Opacity and fragmentation
    2937* [http://adsabs.harvard.edu/abs/1989ApJ...346..336B Boss 1989] Protostellar formation in rotating interstellar clouds. VIII - Inner core formation
     38* [http://adsabs.harvard.edu/abs/1989ApJ...342..834L Shu & Lizano 1989] Molecular cloud cores and bimodal star formation
     39* [http://adsabs.harvard.edu/abs/1991ApJ...373..169M Mouschovias 1991] Magnetic braking, ambipolar diffusion, cloud cores, and star formation - Natural length scales and protostellar masses
     40* [http://adsabs.harvard.edu/abs/1992A%26A...257..715F Falgarone 1992] The small-scale density and velocity structure of quiescent molecular clouds
     41* [http://adsabs.harvard.edu/abs/1992ApJ...391..199F Fiedler & Mouschovias 1992] Ambipolar diffusion and star formation: Formation and contraction of axisymmetric cloud cores. I - Formulation of the problem and method of solution
    3042* [http://adsabs.harvard.edu/abs/1993ApJ...410..157B Boss 1993] Collapse and fragmentation of molecular cloud cores. I - Moderately centrally condensed cores
     43* [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
     44* [http://adsabs.harvard.edu/abs/1993ApJ...416..303F Foster & Chevalier 1993] Gravitational Collapse of an Isothermal Sphere
     45* [http://adsabs.harvard.edu/abs/1993ApJ...417..220G Galli & Shu 1993] Collapse of Magnetized Molecular Cloud Cores. I. Semianalytical Solution
     46* [http://adsabs.harvard.edu/abs/1993ApJ...417..243G Galli & Shu 1993] Collapse of Magnetized Molecular Cloud Cores. II. Numerical Results
     47* [http://adsabs.harvard.edu/abs/1994ApJ...430L..49H Hartmann et al 1994] Protostellar collapse in a self-gravitating sheet
    3148* [http://adsabs.harvard.edu/abs/1995ApJ...439..224B Boss 1995] Collapse and fragmentation of molecular cloud cores. 2: Collapse induced by stellar shock waves
    3249* [http://adsabs.harvard.edu/abs/1995ApJ...451..218B Boss 1995] Collapse and Fragmentation of Molecular Cloud Cores. III. Initial Differential Rotation
    3350* [http://adsabs.harvard.edu/abs/1996ApJ...468..231B Boss 1996] Collapse and Fragmentation of Molecular Cloud Cores. IV. Oblate Clouds and Small Cluster Formation
     51* [http://adsabs.harvard.edu/abs/1996ApJ...462..725G Gammie 1996] Linear Theory of Magnetized, Viscous, Self-gravitating Gas Disks
     52* [http://adsabs.harvard.edu/abs/1996ApJ...466..814G Gammie & Ostriker 1996] Can Nonlinear Hydromagnetic Waves Support a Self-gravitating Cloud?
     53* [http://adsabs.harvard.edu/abs/1996ApJ...464..387H Hartmann et al 1996] Sheet Models of Protostellar Collapse
    3454* [http://adsabs.harvard.edu/abs/1997ApJ...483..309B Boss 1997] Collapse and Fragmentation of Molecular Cloud Cores. V. Loss of Magnetic Field Support
     55* [http://adsabs.harvard.edu/abs/1997ApJ...476..750M McLaughlin & Pudritz 1997] Gravitational Collapse and Star Formation in Logotropic and Nonisothermal Spheres
     56* [http://adsabs.harvard.edu/abs/1997ASPC..123..117P Pudritz et al 1997] Collapse and Outflow: Towards an Integrated Theory of Star Formation
     57* [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
     58* [http://adsabs.harvard.edu/abs/1998ApJ...508L..95B Bate 1998] Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations
     59* [http://adsabs.harvard.edu/abs/1998ApJ...501L.205K Klessen et al 1998] Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster
     60* [http://adsabs.harvard.edu/abs/1998ApJ...495..346M Masunaga et al. 1998] A Radiation Hydrodynamic Model for Protostellar Collapse. I. The First Collapse
     61* [http://adsabs.harvard.edu/abs/1998ApJ...494..587N Nakano 1998] Star Formation in Magnetic Clouds
     62* [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
     63* [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
     64* [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?
    3565* [http://adsabs.harvard.edu/abs/1999ApJ...520..744B Boss 1999] Collapse and Fragmentation of Molecular Cloud Cores. VI. Slowly Rotating Magnetic Clouds
     66* [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
    3667* [http://adsabs.harvard.edu/abs/2000ApJ...528..325B Boss et al 2000] The Jeans Condition and Collapsing Molecular Cloud Cores: Filaments or Binaries?
     68* [http://adsabs.harvard.edu/abs/2000ApJ...535..887K Heitsch et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
     69* [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
     70* [http://adsabs.harvard.edu/abs/2000ApJS..128..287K Klessen et al 2000] The Formation of Stellar Clusters: Gaussian Cloud Conditions. I.x
     71* [http://adsabs.harvard.edu/abs/2000ApJ...535..887K Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
     72* [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
     73* [http://adsabs.harvard.edu/abs/2000AAS...197.0502L Li et al 2000] Simulations of Star Formation out of a Turbulence Molecular Cloud
     74* [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
     75* [http://adsabs.harvard.edu/abs/2001ApJ...552..639A Aikawa et al 2001] Molecular Evolution in Collapsing Prestellar Cores
    3776* [http://adsabs.harvard.edu/abs/2001ApJ...562..842B Boss & Hartmann 2001] Protostellar Collapse in a Rotating, Self-gravitating Sheet
     77* [http://adsabs.harvard.edu/abs/2001ApJ...562..852H Hartmann et al. 2001] Rapid Formation of Molecular Clouds and Stars in the Solar Neighborhood
     78* [http://adsabs.harvard.edu/abs/2001ApJ...547..280H Heitsch et al 2001] Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
     79* [http://adsabs.harvard.edu/abs/2001ApJ...547..280H Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
     80* [http://adsabs.harvard.edu/abs/2001ApJ...556..837K Klessen 2001] The Formation of Stellar Clusters: Mass Spectra from Turbulent Molecular Cloud Fragmentation
     81* [http://adsabs.harvard.edu/abs/2001A%26A...379.1005O Ossenkopf 2001] On the structure of self-gravitating molecular clouds
     82* [http://adsabs.harvard.edu/abs/2001ApJ...546..980O Ostriker 2001] Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models
     83* [http://adsabs.harvard.edu/abs/2002Sci...295...93A Abel et al 2002] The Formation of the First Star in the Universe
    3884* [http://adsabs.harvard.edu/abs/2002ApJ...568..743B Boss 2002] Collapse and Fragmentation of Molecular Cloud Cores. VII. Magnetic Fields and Multiple Protostar Formation
     85* [http://adsabs.harvard.edu/abs/2002ApJ...577..206E Elmegreen 2002] Star Formation from Galaxies to Globules
     86* [http://adsabs.harvard.edu/abs/2002ApJ...576..870P Padoan & Nordlund 2002] The Stellar Initial Mass Function from Turbulent Fragmentation
     87* [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
     88* [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
     89* [http://adsabs.harvard.edu/abs/2003ApJ...592..188B Ballesteros-Paredes 2003] Dynamic cores in hydrostatic disguise
     90 * SPH Turbulent driving of various sorts with self-gravity turned on. (Periodic BC) 205,379 particles
     91* [http://adsabs.harvard.edu/abs/2003MNRAS.340..870H Hennebelle et al. 2003] Protostellar collapse induced by compression
     92* [http://adsabs.harvard.edu/abs/2003RPPh...66.1651L Larson 2003] The physics of star formation
     93* [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
     94* [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
     95* [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
     96* [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
     97* [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
     98* [http://adsabs.harvard.edu/abs/2004MNRAS.348..687H Hennebelle et al. 2004] Protostellar collapse induced by compression - II. Rotation and fragmentation
     99* [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
    39100* [http://adsabs.harvard.edu/abs/2005ApJ...622..393B Boss 2005] Collapse and Fragmentation of Molecular Cloud Cores. VIII. Magnetically Supported Infinite Sheets
     101* [http://adsabs.harvard.edu/abs/2005MNRAS.361....2C Clark and Bonnell 2005] The onset of collapse in turbulently supported molecular clouds
     102* [http://adsabs.harvard.edu/abs/2005ApJ...633L.113H Heitsch et al 2005] Formation of Structure in Molecular Clouds: A Case Study
     103* [http://adsabs.harvard.edu/abs/2005A%26A...435..611J Jappsen et al 2005] The stellar mass spectrum from non-isothermal gravoturbulent fragmentation
     104* [http://adsabs.harvard.edu/abs/2005ApJ...620..786K Klessen et al 2005] Quiescent and Coherent Cores from Gravoturbulent Fragmentation
     105* [http://adsabs.harvard.edu/abs/2005ApJ...618..344V Li et al 2004] The Lifetimes and Evolution of Molecular Cloud Cores
     106* [http://adsabs.harvard.edu/abs/2005ApJ...620L..19L Li et al 2005] Control of Star Formation in Galaxies by Gravitational Instability
     107* [http://adsabs.harvard.edu/abs/2005ApJ...618..344V Vazquez-Semadeni 2005] The Lifetimes and Evolution of Molecular Cloud Cores
     108* [http://adsabs.harvard.edu/abs/2005ApJ...630L..49V Vazquez-Semadeni et al. 2005] Star Formation Efficiency in Driven, Supercritical, Turbulent Clouds
     109* [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
     110* [http://adsabs.harvard.edu/abs/2006MNRAS.372..443B Ballesteros-Paredes 2006] Six myths on the virial theorem for interstellar clouds
     111* [http://adsabs.harvard.edu/abs/2006MNRAS.370..488B Bonnell and Bate 2006] Star formation through gravitational collapse and competitive accretion
     112* [http://adsabs.harvard.edu/abs/2006MNRAS.368.1296B Bonnell and Bate 2006] The Jeans mass and the origin of the knee in the IMF
     113* [http://adsabs.harvard.edu/abs/2006ApJ...648.1052H Heitsch et al 2006] The Birth of Molecular Clouds: Formation of Atomic Precursors in Colliding Flows
     114* [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
     115* [http://adsabs.harvard.edu/abs/2007prpl.conf...63B Ballesteros-Paredes 2007] Molecular Cloud Turbulence and Star Formation
    40116* [http://adsabs.harvard.edu/abs/2007astro.ph..1210B Boss 2007] Collapse and Fragmentation of Molecular Cloud Cores. IX. Magnetic Braking of Initially Filamentary Clouds
     117* [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
     118* [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]
     119* [http://adsabs.harvard.edu/abs/2007arXiv0711.2417H Hennebelle et al 2007] Diffuse interstellar medium and the formation of molecular clouds
     120* [http://adsabs.harvard.edu/abs/2007ApJ...656..959K Krumholz et al 2007] Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores
     121* [http://adsabs.harvard.edu/abs/2007ARA%26A..45..565M McKee Ostriker 2007] Theory of Star Formation
     122* [http://adsabs.harvard.edu/abs/2007MNRAS.377...77P Price & Bate 2007] The impact of magnetic fields on single and binary star formation
     123* [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
     124* [http://adsabs.harvard.edu/abs/2008ApJ...676.1109F Furesz et al. 2008] Kinematic Structure of the Orion Nebula Cluster and its Surroundings
     125* [http://adsabs.harvard.edu/abs/2008ApJ...674..316H Heitsch et al 2008] Cooling, Gravity, and Geometry: Flow-driven Massive Core Formation
     126* [http://adsabs.harvard.edu/abs/2008ApJ...689..290H Heitsch & Hartmann 2008] Rapid Molecular Cloud and Star Formation: Mechanisms and Movies
     127* [http://adsabs.harvard.edu/abs/2008A%26A...486L..43H Hennebelle et al. 2008] From the warm magnetized atomic medium to molecular clouds
     128* [http://adsabs.harvard.edu/abs/2008ApJ...684..395H Hennebelle & Chabrier 2008] Analytical Theory for the Initial Mass Function: CO Clumps and Prestellar Cores
     129* [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
     130 * 128^3^ isothermal MHD with AD and feedback 2.4 pc -> .02 pc
     131 * B=15 microG (beta=1/24) subcritical
     132* [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
     133 * 1100/cc 10K
     134* [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
     135* [http://adsabs.harvard.edu/abs/2008MNRAS.385.1820P Price & Bate 2008] The effect of magnetic fields on star cluster formation
     136* [http://adsabs.harvard.edu/abs/2009MNRAS.398.1082B Banerjee et al 2009] Clump morphology and evolution in MHD simulations of molecular cloud formation
     137* [http://adsabs.harvard.edu/abs/2009ApJ...702.1428H Hennebelle & Chabrier 2009] Analytical Theory for the Initial Mass Function. II. Properties of the Flow
     138* [http://adsabs.harvard.edu/abs/2009ApJ...699.1092H Heyer et al. 2009] Re-Examining Larson's Scaling Relationships in Galactic Molecular Clouds
     139* [http://adsabs.harvard.edu/abs/2009ApJ...693..914O Offner et al 2009] The Shapes of Molecular Cloud Cores in Simulations and Observations
     140* [http://adsabs.harvard.edu/abs/2009MNRAS.398...33P Price & Bate 2009] Inefficient star formation: the combined effects of magnetic fields and radiative feedback
     141* [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
     142* [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
     143* [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
     144* [http://adsabs.harvard.edu/abs/2010ApJ...714L..58T Tomida 2010] Radiation Magnetohydrodynamics Simulation of Proto-stellar Collapse: Two-component Molecular Outflow
     145* [http://adsabs.harvard.edu/abs/2010ApJ...709...27W Wang et al 2010] Outflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster-Forming Clumps
     146* [http://adsabs.harvard.edu/abs/2011MNRAS.411...65B Ballesteros-Paredes 2011] Gravity or turbulence? Velocity dispersion-size relation
     147* [http://adsabs.harvard.edu/abs/2011arXiv1105.5411B Ballesteros-Paredes 2011] Gravity or turbulence? II. Evolving column density PDFs in molecular clouds
    41148* [http://adsabs.harvard.edu/abs/2011MNRAS.410L...8C Cho & Kim 2011] Enhanced core formation rate in a turbulent cloud by self-gravity
    42149 * 512^3^ Isothermal MHD fixed grid
     
    46153 * Power law tail
    47154 * Line-width size relation
    48 * [http://adsabs.harvard.edu/abs/1980ApJ...242..765C Cohn 1980] Late core collapse in star clusters and the gravothermal instability
    49 * [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
    50155* [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
    51 * [http://adsabs.harvard.edu/abs/2005MNRAS.361....2C Clark and Bonnell 2005] The onset of collapse in turbulently supported molecular clouds
    52 * [hhttp://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
     156* [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
    53157 * ENZO 128^3^+4 = 2048^3^; 10pc -> 1000 AU; MHD Isothermal 10K; n=300/cc; B=.6+-2.7 microG (no AD) (supercritical)
    54158 * power law tail for density (1.64) and B (2.74)
     
    56160 * sigma = rho^.25^ for cores
    57161 * CMF = 2.1+-.6
    58 * [http://adsabs.harvard.edu/abs/2002ApJ...577..206E Elmegreen 2002] Star Formation from Galaxies to Globules
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    107165 * Power law tail to density pdf
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    129  * 128^3^ isothermal MHD with AD and feedback 2.4 pc -> .02 pc
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     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
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     210* [http://adsabs.harvard.edu/abs/2011 MNRAS.410L...8C Cho & Kim 2011] Enhanced core formation rate in a turbulent cloud by self-gravity
     211 * 512^3^ Isothermal MHD fixed grid
     212 * beta=.1
     213 * J=4 (l_box/l_jeans)
     214 * M=10
     215 * Power law tail
     216 * 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
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     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
     222 * ENZO 128^3^+4 = 2048^3^; 10pc -> 1000 AU; MHD Isothermal 10K; n=300/cc; B=.6+-2.7 microG (no AD) (supercritical)
     223 * power law tail for density (1.64) and B (2.74)
     224 * B = rho^.48^
     225 * sigma = rho^.25^ for cores
     226 * 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
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     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
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     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
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     336
     337[[CollapsibleEnd]]