Published 1987
| Version v1
Book
Disks and flows around young massive stars
Description
An almost perfect correlation exists between ultracompact HII regions and CO high velocity flows, indicating that dense disks may be confining the flows as claimed in some star formation models. Direct observational data of disks is however very scarce, not only for the massive stars in ultracompact HII regions, but also for the less massive objects
Additional details
Additional titles
- Original title (no language)
- Proto-etoiles et nuages moleculaires.
Publishing Information
- Publisher
- CEA Centre d'Etudes Nucleaires de Saclay.
- Imprint Place
- Gif-sur-Yvette (France)
- Imprint Title
- Protostars and molecular clouds
- Imprint Pagination
- 230 p.
- Journal Page Range
- p. 115-120.
INIS
- Country of Publication
- France
- Country of Input or Organization
- France
- INIS RN
- 19053374
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CARBON MONOXIDE; CONFIGURATION; COSMIC GASES; GAS FLOW; H2 REGIONS; MOLECULES; REVIEWS; STAR EVOLUTION; STARS; VELOCITY
- Descriptors DEC
- CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; COSMIC RADIO SOURCES; DOCUMENT TYPES; FLUID FLOW; FLUIDS; GASES; OXIDES; OXYGEN COMPOUNDS
Optional Information
- Notes
- Imprint:Proto-etoiles et nuages moleculaires.