GRAVITATIONAL FRAGMENTATION IN TURBULENT PRIMORDIAL GAS AND THE INITIAL MASS FUNCTION OF POPULATION III STARS
- 11 January 2011
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 727 (2)
- https://doi.org/10.1088/0004-637x/727/2/110
Abstract
No abstract availableOther Versions
This publication has 102 references indexed in Scilit:
- CHEMICAL EVOLUTION IN HIERARCHICAL MODELS OF COSMIC STRUCTURE. II. THE FORMATION OF THE MILKY WAY STELLAR HALO AND THE DISTRIBUTION OF THE OLDEST STARSThe Astrophysical Journal, 2009
- STAR FORMATION AT VERY LOW METALLICITY. V. THE GREATER IMPORTANCE OF INITIAL CONDITIONS COMPARED TO METALLICITY THRESHOLDSThe Astrophysical Journal, 2009
- Star formation through gravitational collapse and competitive accretionMonthly Notices of the Royal Astronomical Society, 2006
- Thermal Reaction: A Convergence of Theory and ExperimentPhysical Review Letters, 2003
- Collision‐induced Dissociation of Molecular Hydrogen at Low DensitiesThe Astrophysical Journal, 1998
- Radiative and nonradiative charge transfer in+H collisions at low energyPhysical Review A, 1989
- Excitation and dissociation of molecular hydrogen in shock waves at interstellar densitiesThe Astrophysical Journal, 1987
- Gas phase hydrogen atom recombinationSymposium (International) on Combustion, 1975
- Isotope Effect in the Dissociative Attachment inat Low EnergyPhysical Review B, 1967
- A Calculation of the Rates of the Ortho-Para Conversions and Isotope Exchanges in HydrogenThe Journal of Chemical Physics, 1959