Changes between Version 15 and Version 16 of GravoTurbulence


Ignore:
Timestamp:
07/01/11 15:05:28 (14 years ago)
Author:
Jonathan
Comment:

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  • GravoTurbulence

    v15 v16  
    116116* [http://adsabs.harvard.edu/abs/2007astro.ph..1210B Boss 2007] Collapse and Fragmentation of Molecular Cloud Cores. IX. Magnetic Braking of Initially Filamentary Clouds
    117117* [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]
     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
     119* [http://adsabs.harvard.edu/abs/2009Natur.457...63G Goodman et al. 2009] A role for self-gravity at multiple length scales in the process of star formation
    119120* [http://adsabs.harvard.edu/abs/2007arXiv0711.2417H Hennebelle et al 2007] Diffuse interstellar medium and the formation of molecular clouds
    120121* [http://adsabs.harvard.edu/abs/2007ApJ...656..959K Krumholz et al 2007] Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores
    … …  
    239240* [http://adsabs.harvard.edu/abs/1996ApJ...466..814G Gammie & Ostriker 1996] Can Nonlinear Hydromagnetic Waves Support a Self-gravitating Cloud
    240241* [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/2007ApJ...659.1317G Glover & Mac Low 2007] Simulating the Formation of Molecular Clouds. II. Rapid Formation from Turbulent Initial Conditions
     243* [http://adsabs.harvard.edu/abs/2009Natur.457...63G Goodman et al. 2009] A role for self-gravity at multiple length scales in the process of star formation
    242244* [http://adsabs.harvard.edu/abs/1980ApJ...238..991G Goldreich & Weber 1980] Homologously collapsing stellar cores
    243245* [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