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Deep inside low-mass stars
Low-mass stars exhibit, at all stages of their evolution, the signatures of complex physical processes that require challenging modeling beyond standard stellar theory. In this review, we recall the most striking observational evidences that probe the interaction and interdependence of various trans...
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Published in: | arXiv.org 2008-05 |
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creator | Charbonnel, Corinne Talon, Suzanne |
description | Low-mass stars exhibit, at all stages of their evolution, the signatures of complex physical processes that require challenging modeling beyond standard stellar theory. In this review, we recall the most striking observational evidences that probe the interaction and interdependence of various transport processes of chemicals and angular momentum in these objects. We then focus on the impact of atomic diffusion, large scale mixing due to rotation, and internal gravity waves on stellar properties on the main sequence and slightly beyond. |
doi_str_mv | 10.48550/arxiv.0805.4697 |
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language | eng |
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subjects | Angular momentum Astronomical models Diffusion Gravitational waves Gravity waves Low mass stars Organic chemistry Stellar evolution |
title | Deep inside low-mass stars |
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