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Stellar structure and magnetic fields from pre-main sequence to cataclysmic binaries

Abstract:

I review the problem of lithium depletion in pre-Main Sequence (pre-MS) stars, and the curious points of view which accompanied the changes in the results due to the changes in the stellar physics inputs in the last 35 years. Today, the problem of explaining the present solar lithium abundance is reversed with respect to the problem of some years ago: new standard stellar models deplete too much lithium during the pre-MS evolution. We have recently attempted to model the solar pre-MS by inclu...

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Publication status:
Published

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Authors


D'Antona, F More by this author
Volume:
229
Pages:
21-30
Publication date:
2001
URN:
uuid:c67ac748-3c64-4771-bf1d-d61e3b7aa30f
Source identifiers:
21152
Local pid:
pubs:21152
ISBN:
1-58381-061-7

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