Published 1982
| Version v1
Book
On the chemical abundances, evolutionary stage and bolometric magnitude of WR stars
Description
The author comments on 3 problems concerning WR stars: a) are WR stars core hydrogen/core helium burning. b) are WR stars H-poor or do they have normal abundances. c) can we use B.C. for WR stars which are similar as for O stars. (Auth.)
Additional details
Publishing Information
- Publisher
- D. Reidel.
- Imprint Place
- Dordrecht (Netherlands)
- ISBN
- 90-277-1469-X
- Imprint Title
- Wolf-Rayet stars
- Imprint Pagination
- 636 p.
- Journal Issue
- no. 99
- Series
- International astronomical union symposium.
- Journal Page Range
- p. 117-120.
Conference
- Title
- 99. IAU Symposium on Wolf-Rayet stars.
- Dates
- 18 - 22 Sep 1981.
- Place
- Cozumel (Mexico).
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 14735431
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CHEMICAL COMPOSITION; ELEMENT ABUNDANCE; HELIUM; HELIUM BURNING; HYDROGEN; HYDROGEN BURNING; STAR EVOLUTION; WOLF-RAYET STARS
- Descriptors DEC
- ELEMENTS; MAIN SEQUENCE STARS; NONMETALS; QUANTITY RATIO; RARE GASES; STAR BURNING; STARS
Optional Information
- Notes
- Imprint:Includes subject index.