Published 1987
| Version v1
Miscellaneous
Binary evolution
Description
Consideration of mass transfer and mass loss processes allows the explanation of the existence of well determined groups of binaries, such as Algols, cataclysmic variables, massive and low-mass X-ray binaries. The characteristics of these groups are briefly outlined, and evolutionary scenarios are discussed. The importance of detailed observations for advances in evolutionary computations are stressed. It is argued that, although the links between the mentioned groups of binaries and their progenitors is rather well known, the situation is completely different if the detailed evolutionary history for a given system is required. (author). 99 refs
Additional details
Publishing Information
- Imprint Title
- Astrophysics
- Imprint Pagination
- 341 p.
- Journal Page Range
- p. 251-261.
- Report number
- INIS-mf--11450
Conference
- Title
- 10. European regional astronomy meeting of the IAU.
- Dates
- 24-29 Aug 1987.
- Place
- Prague (Czechoslovakia).
INIS
- Country of Publication
- Serbia and Montenegro
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 20047459
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINARY STARS; COSMIC X-RAY SOURCES; ERUPTIVE VARIABLE STARS; MASS TRANSFER; STAR EVOLUTION; SYMBIOTIC STARS; WOLF-RAYET STARS
- Descriptors DEC
- COSMIC RAY SOURCES; MAIN SEQUENCE STARS; STARS; VARIABLE STARS