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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Bibliographic Details
Published in:arXiv.org 2008-05
Main Authors: Charbonnel, Corinne, Talon, Suzanne
Format: Article
Language:English
Subjects:
Angular momentum
Astronomical models
Diffusion
Gravitational waves
Gravity waves
Low mass stars
Organic chemistry
Stellar evolution
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Summary: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.
ISSN:2331-8422
DOI:10.48550/arxiv.0805.4697