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Rotation of Red Giants
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The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
Subject
Modeling, Evolution
Title
Rotation of Red Giants
Date
2015-01-01
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has manifestation of work
http://hub.abes.fr/edp/periodical/eas/2015/volume_7172/issue_2015/eas1571075/m/web
http://hub.abes.fr/edp/periodical/eas/2015/volume_7172/issue_2015/eas1571075/m/print
related by
http://hub.abes.fr/edp/periodical/eas/2015/volume_7172/issue_2015/eas1571075/authorship/1
http://hub.abes.fr/edp/periodical/eas/2015/volume_7172/issue_2015/eas1571075/authorship/5
http://hub.abes.fr/edp/periodical/eas/2015/volume_7172/issue_2015/eas1571075/authorship/3
http://hub.abes.fr/edp/periodical/eas/2015/volume_7172/issue_2015/eas1571075/authorship/4
http://hub.abes.fr/edp/periodical/eas/2015/volume_7172/issue_2015/eas1571075/authorship/2
Author
Kissin, Y.
Thompson, C.
Editor
Lagadec, E.
Lanz T.
Millour F.
Abstract
A new rotation model for post-main sequence stars is proposed. This model quantitatively reproduces core and surface rotation rates of subgiant stars, as well as the core rotation of helium-burning clump stars.
article type
research-article
publisher identifier
eas1571075
Date Copyrighted
2015-01-01
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© EAS, EDP Sciences, 2015
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