| Issue |
A&A
Volume 394, Number 3, November II 2002
|
|
|---|---|---|
| Page(s) | 965 - 969 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361:20021233 | |
| Published online | 21 October 2002 | |
A more powerful evolution model for rotating stars
Yunnan Astronomical Observatory and National Astronomical Observatories, PO Box 110, 650011 Kunming, PR China
Corresponding author: zyr25@hotmail.com
Received:
30
May
2002
Accepted:
1
August
2002
A new one-dimensional rotating stellar evolution model was developed which, distinct from its previous counterparts based on a conservative rotation case or a “shellular rotation” case, made no special assumptions on the distribution of angular velocity inside a rotating star. The results of the evolutionary calculations are presented and compared with the results of previous studies.
Key words: stars: evolution / stars: rotation / stars: Hertzsprung-Russell (HR) and C-M diagrams
© ESO, 2002
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