Published 1985
| Version v1
Journal article
Evolutionary status of AA Doradus: still an enigma?
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