Structure and evolution of the dynamic gas-dust envelopes accompanying massive-star formation

Details Structure and evolution of the dynamic gas-dust envelopes accompanying massive-star formation Structure and evolution of the dynamic gas-dust envelopes accompanying massive-star formation

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..889k&link_type=abstract

Astronomicheskii Zhurnal, Vol. 60, p.889

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The structure and the dynamics of protostellar envelopes are investigated. It is shown that when the stellar core luminosity reaches a certain critical value the collapse is reversed. The dynamics and the stability of the envelopes at this stage and the maximum masses of forming stars depend on the accretion rate. The necessary conditions for massive star formation are considered.

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