Statistics – Computation
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...61i&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, May-June 1987, p. 61-66. In Russian.
Statistics
Computation
1
Computational Astrophysics, Gravitational Collapse, Protostars, Stellar Composition, Stellar Evolution, Abundance, Chemical Composition, Gas Cooling, Hydrogen, Molecular Collisions, Stellar Structure
Scientific paper
A numerical study is carried out of the collapse of protostars which have a primordial chemical composition and are cooled by molecular hydrogen. Consideration is given to the processes governing the formation of H2 molecules during triple collisions. The structure of the protostar at the onset of stellar core formation is determined and the dependence of the protostar's physical characteristics on the initial abundance of molecular hydrogen is analyzed.
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