The formation of first-generation stars. II - Maximum masses of stars

Details The formation of first-generation stars. II - Maximum masses of stars The formation of first-generation stars. II - Maximum masses of stars

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...30i&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, July-Aug. 1987, p. 30-39. In Russian.

Computer Science

Maxima, Protostars, Star Formation, Stellar Mass, Chemical Composition, Hydrogen Clouds, Molecular Clouds, Stellar Envelopes, Stellar Mass Accretion

Scientific paper

The dynamics of protostar envelopes cooled by molecular hydrogen is studied. The main mechanism limiting the accretion of protostar matter onto the stellar core is photodissociation of H2 when the temperature of the star reaches 9000 K. The dependence of the maximum mass of a star with a primordial chemical composition on the initial abundance of molecular hydrogen is obtained.

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