Published January 1977
| Version v1
Journal article
The dynamical evolution of massive protostellar clouds
Creators
- 1. Max-Planck-Institut fuer Physik und Astrophysik, Muenchen (Germany, F.R.)
Description
Dynamical calculations for the envelopes of massive protostars are presented starting from the point when the cloud begins to collapse until the matter in the envelope has become tenuous enough for an H II region to form. (orig./WL)
Abstract (German)
Es werden dynamische Berechnungen fuer die Huellen massiver Protosterne vom Zusammensturz der Wolke bis zur Bildung eines H II-Bereichs in der ausreichend duenn gewordenen Materie der Huelle vorgelegt. (orig./WL)Additional details
Publishing Information
- Journal Title
- Astron. Astrophys.
- Journal Volume
- 54
- Journal Issue
- 1
- Series
- Astron. Astrophys.
- Journal Page Range
- 183-194
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 8333778
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC DUST; COSMIC GASES; H2 REGIONS; NEBULAE; PROTOSTARS; RADIATION TRANSPORT; STAR ACCRETION; STAR EVOLUTION
- Descriptors DEC
- COSMIC RADIO SOURCES; DUSTS; FLUIDS; GASES
Optional Information
- Notes
- 9 figs.; 27 refs.