Published 1985 | Version v1
Journal article

Evolutionary status of AA Doradus: still an enigma?

Creators

  • 1. Polska Akademia Nauk, Warsaw (Poland). Centrum Astronomiczne

Description

The evolutionary scenarios for AA Dor are reconsidered using new contraction times for degenerate red dwarfs. It is found that both types of models considered by Paczynski (1980) with the primary being either an hydrogen shell burning helium white dwarf or a double shell burning carbon-oxygen white dwarf are consistent with the available data. The second model requires a very narrow range of the initial parameters of the binary system. 26 refs. (author)

Additional details

Publishing Information

Journal Title
Acta Astronomica
Journal Volume
35
Journal Issue
1-2
Series
Acta Astron.
Journal Page Range
97-107
ISSN
0001-5237
CODEN
AASWA

INIS

Country of Publication
Poland
Country of Input or Organization
Poland
INIS RN
20082096
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BINARY STARS; HELIUM BURNING; RED DWARF STARS; STAR EVOLUTION; STAR MODELS; WHITE DWARF STARS
Descriptors DEC
DWARF STARS; MATHEMATICAL MODELS; STAR BURNING; STARS