SIMULATIONS ON A MOVING MESH: THE CLUSTERED FORMATION OF POPULATION III PROTOSTARS
暂无分享,去创建一个
Volker Springel | Volker Bromm | Paul Clark | Ralf Klessen | Simon Glover | R. Klessen | S. Glover | S. White | V. Springel | T. Greif | V. Bromm | P. Clark | Simon White | Thomas Greif | Rowan Smith | Rowan J. Smith | S. White
[1] R. Klessen,et al. THE FORMATION OF STELLAR CLUSTERS: GAUSSIAN CLOUD CONDITIONS. I , 2022 .
[2] I. A. Bonnell,et al. Modelling accretion in protobinary systems , 1995 .
[3] R. Klessen,et al. The Formation and Fragmentation of Disks Around Primordial Protostars , 2011, Science.
[4] P. Bodenheimer,et al. Stellar Structure of Dark Stars: A First Phase of Stellar Evolution Resulting from Dark Matter Annihilation , 2008, 0806.0617.
[5] D. Flower,et al. Three‐body recombination of hydrogen during primordial star formation , 2007 .
[6] P. Bodenheimer,et al. Fragmentation in a rotating protostar - A comparison of two three-dimensional computer codes , 1979 .
[7] T. Beers,et al. THE DISCOVERY AND ANALYSIS OF VERY METAL-POOR STARS IN THE GALAXY , 2005 .
[8] Formation of Primordial Stars in a ΛCDM Universe , 2006, astro-ph/0606106.
[9] D. H. Schwarz,et al. Master Equation Studies of the Collisional Excitation and Dissociation of H 2 Molecules by H Atoms , 1996 .
[10] R. Klessen,et al. GRAVITATIONAL FRAGMENTATION IN TURBULENT PRIMORDIAL GAS AND THE INITIAL MASS FUNCTION OF POPULATION III STARS , 2010, 1006.1508.
[11] David A. Neufeld,et al. Radiative Cooling of Warm Molecular Gas , 1993 .
[12] U. California,et al. The distribution and kinematics of early high-σ peaks in present-day haloes: implications for rare objects and old stellar populations , 2005, astro-ph/0506615.
[13] A. Loeb,et al. Rotation Speed of the First Stars , 2010, 1010.0997.
[14] Michael L. Norman,et al. The Formation of the First Star in the Universe , 2001, Science.
[15] I. McGreer,et al. The Impact of HD Cooling on the Formation of the First Stars , 2008, 0802.3918.
[16] Pisa,et al. First star formation with dark matter annihilation , 2010, 1003.0676.
[17] A. Bressan,et al. Dark matter annihilation effects on the first stars , 2008, 0805.4016.
[18] K. Nomoto,et al. Nucleosynthesis of Zinc and Iron Peak Elements in Population III Type II Supernovae: Comparison with Abundances of Very Metal Poor Halo Stars , 2001, astro-ph/0103241.
[19] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE * OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[20] The First Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars , 2005, Science.
[21] B. O’Shea,et al. Population III Star Formation in a ΛCDM Universe. I. The Effect of Formation Redshift and Environment on Protostellar Accretion Rate , 2006, astro-ph/0607013.
[22] Volker Bromm,et al. The Formation of the First Stars. I. The Primordial Star-forming Cloud , 2002 .
[23] P. Bodenheimer,et al. Multiple fragmentation in collapsing protostars , 1993 .
[24] M. Bate,et al. Resolution requirements for smoothed particle hydrodynamics calculations with self-gravity , 1997 .
[26] J. Monaghan,et al. Fundamental differences between SPH and grid methods , 2006, astro-ph/0610051.
[27] Abraham Loeb,et al. In the Beginning: The First Sources of Light and the Reionization of the Universe , 2000 .
[28] Accretion onto a primordial protostar , 2003, astro-ph/0312456.
[29] R. Klein,et al. The Formation of Massive Star Systems by Accretion , 2009, Science.
[30] R. Klessen,et al. MODELING COLLAPSE AND ACCRETION IN TURBULENT GAS CLOUDS: IMPLEMENTATION AND COMPARISON OF SINK PARTICLES IN AMR AND SPH , 2010, 1001.4456.
[31] Volker Bromm,et al. The formation of a star cluster: predicting the properties of stars and brown dwarfs , 2002, astro-ph/0212380.
[32] R. Klessen,et al. The First Stellar Cluster , 2007, 0706.0613.
[33] Embedding Lagrangian Sink Particles in Eulerian Grids , 2003, astro-ph/0312612.
[34] K. Omukai,et al. EVOLUTION OF MASSIVE PROTOSTARS WITH HIGH ACCRETION RATES , 2008, 0806.4122.
[35] V. Springel. E pur si muove: Galilean-invariant cosmological hydrodynamical simulations on a moving mesh , 2009, 0901.4107.
[36] J. Monaghan. Smoothed particle hydrodynamics , 2005 .
[37] Simulations of Pregalactic Structure Formation with Radiative Feedback , 2000, astro-ph/0007198.
[38] M. Norman,et al. HIGH-ENTROPY POLAR REGIONS AROUND THE FIRST PROTOSTARS , 2010, 1010.6076.
[39] How small were the first cosmological objects , 1996, astro-ph/9603007.
[40] T. Greif,et al. The first stars: formation of binaries and small multiple systems , 2009, 0908.0712.
[41] V. Springel,et al. The first generation of stars in the Λ cold dark matter cosmology , 2006, astro-ph/0610174.
[42] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[43] R. Klessen,et al. H II REGIONS: WITNESSES TO MASSIVE STAR FORMATION , 2010, 1001.2470.
[44] H. Zinnecker,et al. Toward Understanding Massive Star Formation , 2007, 0707.1279.
[45] C. McKee,et al. The Formation of the First Stars. II. Radiative Feedback Processes and Implications for the Initial Mass Function , 2007, 0711.1377.
[46] New Haven,et al. The Stellar Mass Spectrum from Non-Isothermal Gravoturbulent Fragmentation , 2004, astro-ph/0410351.
[47] Matthew J. Turk,et al. The Formation of Population III Binaries from Cosmological Initial Conditions , 2009, Science.
[48] R. Klessen,et al. EFFECTS OF VARYING THE THREE-BODY MOLECULAR HYDROGEN FORMATION RATE IN PRIMORDIAL STAR FORMATION , 2010, 1011.1908.
[49] Rosseland and Planck mean opacities for primordial matter , 2004, astro-ph/0411613.
[50] R. Klessen,et al. Control of star formation by supersonic turbulence , 2000, astro-ph/0301093.
[51] V. Springel. Smoothed Particle Hydrodynamics in Astrophysics , 2010, 1109.2219.
[52] E. Ripamonti. The role of HD cooling in primordial star formation , 2007, astro-ph/0701148.
[53] K. Omukai,et al. Formation of Primordial Protostars , 1998, astro-ph/9811308.
[54] S. E. Woosley,et al. The Nucleosynthetic Signature of Population III , 2002 .
[55] T. Abel,et al. Uncertainties in H2 and HD chemistry and cooling and their role in early structure formation , 2008, 0803.1768.
[56] Fragmentation and the formation of primordial protostars: the possible role of collision-induced emission , 2003, astro-ph/0311355.
[57] Cosmological Formation of Low-Mass Objects , 1995, astro-ph/9507111.
[58] Lars Hernquist,et al. Protostar Formation in the Early Universe , 2008, Science.
[59] Edward J. Wollack,et al. FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.
[60] A. Frebel,et al. The minimum stellar metallicity observable in the Galaxy , 2008, 0811.0020.
[61] Radiation from the first forming stars , 2001, astro-ph/0107095.
[62] E. Ostriker,et al. Theory of Star Formation , 2007, 0707.3514.
[63] Richard I. Klein,et al. Self-gravitational Hydrodynamics with Three-dimensional Adaptive Mesh Refinement: Methodology and Applications to Molecular Cloud Collapse and Fragmentation , 1998 .
[64] N. Yoshida,et al. LOW-METALLICITY STAR FORMATION: PRESTELLAR COLLAPSE AND PROTOSTELLAR ACCRETION IN THE SPHERICAL SYMMETRY , 2010, 1008.4262.
[65] Simulations of Early Structure Formation: Primordial Gas Clouds , 2003, astro-ph/0301645.
[66] E. Salpeter,et al. Primordial stellar evolution - The protostar phase , 1986 .
[67] T. Greif,et al. The First Stars , 2003, astro-ph/0311019.
[68] V. Springel,et al. The earliest stars and their relics in the Milky Way , 2009, 0909.1593.
[69] S. Kitsionas,et al. Smoothed Particle Hydrodynamics with particle splitting, applied to self-gravitating collapse , 2002, astro-ph/0203057.
[70] N. Yoshida,et al. The formation of the first stars and galaxies , 2009, Nature.