Changes between Version 7 and Version 8 of GravoTurbulence


Ignore:
Timestamp:
07/01/11 11:05:21 (14 years ago)
Author:
Jonathan
Comment:

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  • GravoTurbulence

    v7 v8  
    22
    33== References ==
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    … …  
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    … …  
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    4848 * ENZO 128^3^+4 = 2048^3^; 10pc -> 1000 AU; MHD Isothermal 10K; n=300/cc; B=.6+-2.7 microG (no AD) (supercritical)
    … …  
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    109109* [http://adsabs.harvard.edu/abs/1997ApJ...476..750M McLaughlin & Pudritz 1997] Gravitational Collapse and Star Formation in Logotropic and Nonisothermal Spheres
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    … …  
    117117 * B=15 microG (beta=1/24) subcritical
    118118* [http://adsabs.harvard.edu/abs/1998ApJ...494..587N Nakano 1998] Star Formation in Magnetic Clouds
    119 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ApJ...686.1174O&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Offner et al 2008]
     119* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ApJ...686.1174O&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Offner et al 2008] Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars
    120120 * 1100/cc 10K
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    122 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ApJ...693..914O&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Offner et al 2009]
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