On the variation of specific angular momentum among Main Sequence stars
β Scribed by S. P. Tarafdar; M. S. Vardya
- Publisher
- Springer Netherlands
- Year
- 1971
- Tongue
- English
- Weight
- 677 KB
- Volume
- 13
- Category
- Article
- ISSN
- 0004-640X
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π SIMILAR VOLUMES
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 A marked seasonal variation of the poleward angularβmomentum flux for the northern hemisphere in the vicinity of 30Β°N. latitude is obtained from an analysis of upperβwind soundings for a period of one year. The angularβmomentum flux appears to be about twice as great during the winter a