Is Core Angular Momentum Key to the Giant Dynamo?
The pros and cons of core angular momentum dissipation into the convective envelopes of giants as a driver of giant activity is discussed in face of the observational evidence, which points to two ”magnetic strips“, in the HRD, where in the first, at the base of the RGB, activity of moderate mass st...
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| Main Authors: | , |
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| Format: | Artigo |
| Language: | Inglês |
| Published: |
MDPI AG
2022-08-01
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| Series: | Universe |
| Subjects: | |
| Online Access: | https://www.mdpi.com/2218-1997/8/8/411 |
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