Changes between Version 6 and Version 7 of GravoTurbulence


Ignore:
Timestamp:
06/30/11 17:31:31 (14 years ago)
Author:
Jonathan
Comment:

—

Legend:

Unmodified
Added
Removed
Modified

  • GravoTurbulence

    v6 v7  
    8181* [http://adsabs.harvard.edu/abs/2008ApJ...684..395H hennebelle & Chabrier 2008] Analytical Theory for the Initial Mass Function: CO Clumps and Prestellar Cores
    8282* [http://adsabs.harvard.edu/abs/2009ApJ...702.1428H Hennebelle & Chabrier 2009] Analytical Theory for the Initial Mass Function. II. Properties of the Flow
     83* [http://adsabs.harvard.edu/abs/2011arXiv1101.4940H Hopkins et al 2011] Self-Regulated Star Formation in Galaxies via Momentum Input from Massive Stars
    8384* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ApJ...699.1092H&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Heyer et al. 2009]
    8485* [http://adsabs.harvard.edu/abs/1998ApJ...501L.205K Klessen et al 1998] Fragmentation of Molecular Clouds: The Initial Phase of a Stellar Cluster
     86* [http://adsabs.harvard.edu/abs/1986ApJ...305..309H Hunter et al 1986] Star formation in colliding gas flows
     87* [http://adsabs.harvard.edu/abs/2005A%26A...435..611J Jappsen et al 2005] The stellar mass spectrum from non-isothermal gravoturbulent fragmentation
    8588* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ApJ...556..837K&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Klessen 2001]
    86 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ApJS..128..287K&db_key=AST&link_type=ABSTRACT Klessen et al 2000]
    87 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ApJ...535..887K&db_key=AST&link_type=ABSTRACT Klessen et al 2000]
     89* [http://adsabs.harvard.edu/abs/2000ApJS..128..287K Klessen et al 2000] The Formation of Stellar Clusters: Gaussian Cloud Conditions. I.x
     90* [http://adsabs.harvard.edu/abs/2000ApJ...535..887K Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. I. Gasdynamical Turbulence
     91* [http://adsabs.harvard.edu/abs/2001ApJ...547..280H Klessen et al 2000] Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical Turbulence
     92* [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
     93* [http://adsabs.harvard.edu/abs/2005ApJ...620..786K Klessen et al 2005] Quiescent and Coherent Cores from Gravoturbulent Fragmentation
    8894* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ApJ...727L..20K&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Kritsuk et al 2011]
    8995 * ENZO 512^3^+5x2=524,288^3^; 5pc -> 2 AU; Isothermal 10K; n=500/cc
    9096 * Power law tail to density pdf
     97* [http://adsabs.harvard.edu/abs/2007ApJ...656..959K Krumholz et al 2007] Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores
     98* [http://adsabs.harvard.edu/abs/2011ApJ...731...25K Krumholz et al 2011] Which Phase of the Interstellar Medium Correlates with the Star Formation Rate?
     99* [http://adsabs.harvard.edu/abs/1981MNRAS.194..809L Larson 1981] Turbulence and star formation in molecular clouds
     100* [http://adsabs.harvard.edu/abs/1985MNRAS.214..379L Larson 1985] Cloud fragmentation and stellar masses
     101* [http://adsabs.harvard.edu/abs/2003RPPh...66.1651L Larson 2003] The physics of star formation
    91102* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ApJ...618..344V&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Li et al 2004]
     103* [http://adsabs.harvard.edu/abs/2000AAS...197.0502L Li et al 2000] Simulations of Star Formation out of a Turbulence Molecular Cloud
     104* [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
     105* [http://adsabs.harvard.edu/abs/2005ApJ...620L..19L Li et al 2005] Control of Star Formation in Galaxies by Gravitational Instability
     106* [http://adsabs.harvard.edu/abs/1965ApJ...142.1431L Lin et al 1965] The Gravitational Collapse of a Uniform Spheroid.
     107* [http://adsabs.harvard.edu/abs/1976MNRAS.176..367L Low & Lyndin-Bell] The minimum Jeans mass or when fragmentation must stop
    92108* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ARA%26A..45..565M&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 McKee Ostriker 2007]
     109* [http://adsabs.harvard.edu/abs/1997ApJ...476..750M McLaughlin & Pudritz 1997] Gravitational Collapse and Star Formation in Logotropic and Nonisothermal Spheres
     110* [http://adsabs.harvard.edu/abs/1984ApJ...279..621M Miyama et al 1984] Criteria for collapse and fragmentation of rotating, isothermal clouds
     111* [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
     112* [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 - Results
     113* [http://adsabs.harvard.edu/abs/1976ApJ...210..326M Mouschovias & Spitzer 1976] Note on the collapse of magnetic interstellar clouds
     114* [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
    93115* [http://adsabs.harvard.edu/abs/2008ApJ...687..354N Nakamura & Li 2008]
    94116 * 128^3^ isothermal MHD with AD and feedback 2.4 pc -> .02 pc
    95117 * B=15 microG (beta=1/24) subcritical
     118* [http://adsabs.harvard.edu/abs/1998ApJ...494..587N Nakano 1998] Star Formation in Magnetic Clouds
    96119* [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]
    97120 * 1100/cc 10K
    … …  
    99122* [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]
    100123* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001A%26A...379.1005O&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Ossenkopf 2001]
    101 * [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ApJ...214..488S&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Shu 77]
     124* [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
     125* [http://adsabs.harvard.edu/abs/2001ApJ...546..980O Ostriker 2001] Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models
     126* [http://adsabs.harvard.edu/abs/2011ApJ...730...40P Padoan & Nordlund 2011] The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence
     127* [http://adsabs.harvard.edu/abs/2002ApJ...576..870P Padoan & Nordlund 2002] The Stellar Initial Mass Function from Turbulent Fragmentation
     128* [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
     129* [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
     130* [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
     131* [http://adsabs.harvard.edu/abs/2007MNRAS.377...77P Price & Bate 2007] The impact of magnetic fields on single and binary star formation
     132* [http://adsabs.harvard.edu/abs/2008MNRAS.385.1820P Price & Bate 2008] The effect of magnetic fields on star cluster formation
     133* [http://adsabs.harvard.edu/abs/2009MNRAS.398...33P Price & Bate 2009] Inefficient star formation: the combined effects of magnetic fields and radiative feedback
     134* [http://adsabs.harvard.edu/abs/1997ASPC..123..117P Pudritz et al 1997] Collapse and Outflow: Towards an Integrated Theory of Star Formation
     135* [http://adsabs.harvard.edu/abs/1977MNRAS.179..541R Rees & Ostriker 1977] Cooling, dynamics and fragmentation of massive gas clouds - Clues to the masses and radii of galaxies and clusters
     136* [http://adsabs.harvard.edu/abs/1977ApJ...214..488S Shu 1977] Self-similar collapse of isothermal spheres and star formation
     137* [http://adsabs.harvard.edu/abs/1987ARA%26A..25...23S Shu, Adams, & Lizano 1987] Star formation in molecular clouds - Observation and theory
    102138* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ApJ...342..834L&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Shu & Lizano 1989]
     139* [http://adsabs.harvard.edu/abs/1966MNRAS.132..359S Strittmatter 1966] Gravitational collapse in the presence of a magnetic field
    103140* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ApJ...286..529T&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Tereby, Shu, & Cassen 1984]
     141* [http://adsabs.harvard.edu/abs/2010ApJ...714L..58T Tomida 2010] Radiation Magnetohydrodynamics Simulation of Proto-stellar Collapse: Two-component Molecular Outflow
    104142* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ApJ...489L.179T&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Truelove 1997]
    105143* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ApJ...495..821T&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Truelove et al. 1998]
    106144* [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
    107 
    108145* [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
    109 
     146* [http://adsabs.harvard.edu/abs/2005ApJ...618..344V Vazquez-Semadeni 2005] The Lifetimes and Evolution of Molecular Cloud Cores
     147* [http://adsabs.harvard.edu/abs/2005ApJ...630L..49V Vazquez-Semadeni et al. 2005] Star Formation Efficiency in Driven, Supercritical, Turbulent Clouds
    110148* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ApJ...643..245V&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Vazques-Semadeni et al 2006]
    111149* [http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ApJ...657..870V&db_key=AST&link_type=ABSTRACT&high=4dd2954bad03054 Vazques-Semadeni et al 2007]