Published May 1985
| Version v1
Journal article
On initial masses of stars, that become Wolf-Rayet stars
Description
It is shown that the spatial distribution and number ratio of massive O and B stars, found by Conti et al., is consistent with the statement, that Wolf-Rayet stars are produced by components of close binaries with Nsub(1.2) γte or approximately 20 Msub(sum) and by all other stars with M > or approximately 40 Msub(sum)
Additional details
Additional titles
- Original title (Russian)
- О начальных массах звезд, превращающихся в звезды Вольфа-Райе
Publishing Information
- Journal Title
- Astron. Zh.
- Journal Volume
- 62
- Journal Issue
- 3
- Series
- Astron. Zh.
- Journal Page Range
- 604-605
- ISSN
- 0004-6299
- CODEN
- ASZHA
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 17014716
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BINARY STARS; MASS; STAR EVOLUTION; WOLF-RAYET STARS
- Descriptors DEC
- MAIN SEQUENCE STARS; STARS
Optional Information
- Notes
- For English translation see the journal Soviet Astronomy (USA).