A note on star formation by gravitational fragmentation

Details A note on star formation by gravitational fragmentation A note on star formation by gravitational fragmentation

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52..662s&link_type=abstract

Astronomicheskii Zhurnal, vol. 52, May-June 1975, p. 662-664. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Gravitational Collapse, Star Formation, Cooling, Early Stars, Fragmentation, Rarefied Gases, Stellar Mass

Scientific paper

The possibility of star formation by gravitational fragmentation is
considered. There is a lower limit for the mass of a fragment, which is
defined by the cooling mechanism and opacity. The minimum mass obtained
coincides with the stellar mass for the contemporary conditions as well
as for ones for the formation of stars of the first generation.

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