๐”– Bobbio Scriptorium
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Angular momentum evolution of lower main sequence stars

โœ Scribed by C. Trigilio; S. Catalano; E. Marilli


Publisher
Elsevier Science
Year
1986
Tongue
English
Weight
184 KB
Volume
6
Category
Article
ISSN
0273-1177

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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

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