Main sequence for rotating stars of intermediate mass
✍ Scribed by D. Eryurt-Ezer; H. Kirbiyik; N. Özkara
- Publisher
- Springer Netherlands
- Year
- 1986
- Tongue
- English
- Weight
- 882 KB
- Volume
- 126
- Category
- Article
- ISSN
- 0004-640X
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Pre-Main-Sequence stars with masses between 2 and 5 M e (Herbig Ae/Be stars) have radiative subphotospheric envelopes. However, they possess strong stellar winds and show definite signs of activity which could be linked to surface magnetic field. Therefore, they must lose angular momentum at a signi
## Abstract ZAMS models with internal differential rotation are computed for 6.5 M~⊙~ and 10 M~⊙~ models with the 2D evolution code ROTORC. Two applications of these models, their pulsational frequencies and deduced locations in the HR diagram, are discussed in order to show how the internal differ