## Abstract We compute the differential rotation of main sequence stars of the spectral types F, G, K, and M by solving the equation of motion and the equation of convective heat transport in a meanβfield formulation. For each spectral type the rotation rate is varied to study the dependence of the
Stellar activity on the lower main sequence in Praesepe
β Scribed by S. Kafka; R.K. Honeycutt
- Publisher
- John Wiley and Sons
- Year
- 2004
- Tongue
- English
- Weight
- 169 KB
- Volume
- 325
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
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