Published 1982
| Version v1
Book
WR stars with ring nebulae
Description
It is shown that most of usually apparently single nitrogen WR stars with ring emission nebulae around them (WN + Neb) are a probable product of the evolution of a massive close binary with initial masses of components exceeding approximately 20 solar masses. (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. 485-489.
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
- 14735480
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINARY STARS; MASS; NEBULAE; STAR EVOLUTION; STELLAR WINDS; VELOCITY; WOLF-RAYET STARS
- Descriptors DEC
- MAIN SEQUENCE STARS; STARS
Optional Information
- Notes
- Imprint:Includes subject index.