Fragmentation of a nonisothermal protostellar cloud

Details Fragmentation of a nonisothermal protostellar cloud Fragmentation of a nonisothermal protostellar cloud

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...55..181b&link_type=abstract

Icarus (ISSN 0019-1035), vol. 55, July 1983, p. 181-184. NASA-supported research.

Other

3

Binary Stars, Interstellar Matter, Protostars, Collapse, Nebulae

Scientific paper

The collapse of a very low thermal energy, rotating cloud results in
fragmentation to a binary protostellar system even in the nonisothermal
regime. The solar system therefore probably did not form from a
fragmentation hierarchy involving ejection of the presolar nebula from a
multiple system.

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