Changes between Version 4 and Version 5 of GravoTurbulence


Ignore:
Timestamp:
06/29/11 12:15:09 (14 years ago)
Author:
Jonathan
Comment:

Legend:

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  • GravoTurbulence

    v4 v5  
    1414* [http://adsabs.harvard.edu/abs/2009MNRAS.398.1082B Banerjee et al 2009] Clump morphology and evolution in MHD simulations of molecular cloud formation
    1515* [http://adsabs.harvard.edu/abs/1998ApJ...508L..95B Bate 1998] Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations
    16 
     16* [http://adsabs.harvard.edu/abs/1987A%26A...172..293B Bonazzola et al, 1987] Jeans collapse in a turbulent medium
     17* [http://adsabs.harvard.edu/abs/2006MNRAS.370..488B Bonnell and Bate 2006] Star formation through gravitational collapse and competitive accretion
     18* [http://adsabs.harvard.edu/abs/2006MNRAS.368.1296B Bonnell and Bate 2006] The Jeans mass and the origin of the knee in the IMF
     19* [http://adsabs.harvard.edu/abs/1980ApJ...236..619B Boss 1980] Protostellar formation in rotating interstellar clouds. I - Numerical methods and tests
     20* [http://adsabs.harvard.edu/abs/1980ApJ...237..563B Boss 1980] Protostellar formation in rotating interstellar clouds. II - Axially symmetric collapse
     21* [http://adsabs.harvard.edu/abs/1980ApJ...237..866B Boss 1980] Protostellar formation in rotating interstellar clouds. III - Nonaxisymmetric collapse
     22* [http://adsabs.harvard.edu/abs/1984ApJ...277..768B Boss 1984] Protostellar formation in rotating interstellar clouds. IV Nonisothermal collapse
     23* [http://adsabs.harvard.edu/abs/1986ApJS...62..519B Boss 1986] Protostellar formation in rotating interstellar clouds. V - Nonisothermal collapse and fragmentation
     24* [http://adsabs.harvard.edu/abs/1987ApJ...319..149B Boss 1987] Protostellar formation in rotating interstellar clouds. VI - Nonuniform initial conditions
     25* [http://adsabs.harvard.edu/abs/1988ApJ...331..370B Boss 1988] Protostellar formation in rotating interstellar clouds. VII - Opacity and fragmentation
     26* [http://adsabs.harvard.edu/abs/1989ApJ...346..336B Boss 1989] Protostellar formation in rotating interstellar clouds. VIII - Inner core formation
     27* [http://adsabs.harvard.edu/abs/1993ApJ...410..157B Boss 1993] Collapse and fragmentation of molecular cloud cores. I - Moderately centrally condensed cores
     28* [http://adsabs.harvard.edu/abs/1995ApJ...439..224B Boss 1995] Collapse and fragmentation of molecular cloud cores. 2: Collapse induced by stellar shock waves
     29* [http://adsabs.harvard.edu/abs/1995ApJ...451..218B Boss 1995] Collapse and Fragmentation of Molecular Cloud Cores. III. Initial Differential Rotation
     30* [http://adsabs.harvard.edu/abs/1996ApJ...468..231B Boss 1996] Collapse and Fragmentation of Molecular Cloud Cores. IV. Oblate Clouds and Small Cluster Formation
     31* [http://adsabs.harvard.edu/abs/1997ApJ...483..309B Boss 1997] Collapse and Fragmentation of Molecular Cloud Cores. V. Loss of Magnetic Field Support
     32* [http://adsabs.harvard.edu/abs/1999ApJ...520..744B Boss 1999] Collapse and Fragmentation of Molecular Cloud Cores. VI. Slowly Rotating Magnetic Clouds
     33* [http://adsabs.harvard.edu/abs/2002ApJ...568..743B Boss 2002] Collapse and Fragmentation of Molecular Cloud Cores. VII. Magnetic Fields and Multiple Protostar Formation
     34* [http://adsabs.harvard.edu/abs/2005ApJ...622..393B Boss 2005] Collapse and Fragmentation of Molecular Cloud Cores. VIII. Magnetically Supported Infinite Sheets
     35* [http://adsabs.harvard.edu/abs/2007astro.ph..1210B Boss 2007] Collapse and Fragmentation of Molecular Cloud Cores. IX. Magnetic Braking of Initially Filamentary Clouds
    1736* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011MNRAS.410L...8C&db_key=AST&link_type=ABSTRACT Cho & Kim 2011]
    1837 * 512^3^ Isothermal MHD fixed grid
     
    2241 * Power law tail
    2342 * Line-width size relation
     43* [http://adsabs.harvard.edu/abs/1980ApJ...242..765C Cohn 1980] Late core collapse in star clusters and the gravothermal instability
     44* [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
    2445* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005MNRAS.361....2C&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Clark and Bonnell 2005]
    2546* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ApJ...731...59C&db_key=AST&link_type=ABSTRACT Collins et al 2011]
     
    2950 * sigma = rho^.25^ for cores
    3051 * CMF = 2.1+-.6
     52* [http://adsabs.harvard.edu/abs/2002ApJ...577..206E Elmegreen 2002] Star Formation from Galaxies to Globules
     53* [http://adsabs.harvard.edu/abs/1992A%26A...257..715F Falgarone 1992] The small-scale density and velocity structure of quiescent molecular clouds
     54* [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
     55* [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
     56* [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
     57* [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
     58* [http://adsabs.harvard.edu/abs/1993ApJ...416..303F Foster & Chevalier 1993] Gravitational Collapse of an Isothermal Sphere
    3159* [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]
    3260* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ApJ...547..280H&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Heitsch et al 2001]