Published 1984
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Evolution of massive stars
Description
The evolution of stars with masses larger than 15 sun masses is reviewed. These stars have large convective cores and lose a substantial fraction of their matter by stellar wind. The treatment of convection and the parameterisation of the stellar wind mass loss are analysed within the context of existing disagreements between theory and observation. The evolution of massive close binaries and the origin of Wolf-Rayet Stars and X-ray binaries is also sketched. (author)
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Additional details
Publishing Information
- Imprint Title
- Spectral evolution of galaxies. Rutherford Appleton Laboratory workshop on astronomy and astrophysics, Abingdon, 23-25 May 1983
- Imprint Pagination
- 210 p.
- Journal Page Range
- p. 1-27.
- Report number
- RAL--84-008
Conference
- Title
- Spectral evolution of galaxies. RAL workshop on astronomy and astrophysics.
- Dates
- 23-25 May 1983.
- Place
- Abingdon (UK).
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 15045322
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINARY STARS; CONVECTION; MASS; REVIEWS; STAR EVOLUTION; STAR MODELS; STELLAR WINDS; WOLF-RAYET STARS
- Descriptors DEC
- DOCUMENT TYPES; ENERGY TRANSFER; HEAT TRANSFER; MAIN SEQUENCE STARS; MATHEMATICAL MODELS; STARS