Published 1987 | Version v1
Miscellaneous

Binary evolution

  • 1. Brussels Univ. (Belgium). Inst. d'Astronomie et d'Astrophysique

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

Part of:
Astrophysics

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

Optional Information