Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantities
Thermohaline mixing has been recently identified as the probable dominating process that governs the photospheric composition of low-mass bright red giant stars. Here, we present the predictions of stellar models computed with the code STAREVOL including this process together with rotational mixing....
Main Authors: | , , , , , |
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Format: | Article |
Language: | English |
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EDP Sciences
2013-03-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20134301006 |
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author | Ekström S. Decressin T. Charbonnel C. Eggenberger P. Lagarde N. Palacios A. |
author_facet | Ekström S. Decressin T. Charbonnel C. Eggenberger P. Lagarde N. Palacios A. |
author_sort | Ekström S. |
collection | DOAJ |
description | Thermohaline mixing has been recently identified as the probable dominating process that governs the photospheric composition of low-mass bright red giant stars. Here, we present the predictions of stellar models computed with the code STAREVOL including this process together with rotational mixing. We compare our theoretical predictions with recent observations, and discuss the effects of both mechanisms on asteroseismic diagnostics. |
first_indexed | 2024-12-20T17:14:01Z |
format | Article |
id | doaj.art-7cc633d0914044e5a5590e9b213f254e |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-12-20T17:14:01Z |
publishDate | 2013-03-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
spelling | doaj.art-7cc633d0914044e5a5590e9b213f254e2022-12-21T19:32:03ZengEDP SciencesEPJ Web of Conferences2100-014X2013-03-01430100610.1051/epjconf/20134301006Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantitiesEkström S.Decressin T.Charbonnel C.Eggenberger P.Lagarde N.Palacios A.Thermohaline mixing has been recently identified as the probable dominating process that governs the photospheric composition of low-mass bright red giant stars. Here, we present the predictions of stellar models computed with the code STAREVOL including this process together with rotational mixing. We compare our theoretical predictions with recent observations, and discuss the effects of both mechanisms on asteroseismic diagnostics.http://dx.doi.org/10.1051/epjconf/20134301006 |
spellingShingle | Ekström S. Decressin T. Charbonnel C. Eggenberger P. Lagarde N. Palacios A. Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantities EPJ Web of Conferences |
title | Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantities |
title_full | Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantities |
title_fullStr | Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantities |
title_full_unstemmed | Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantities |
title_short | Thermohaline instability and rotation-induced mixing in low and intermediate mass stars: Consequences on global asteroseismic quantities |
title_sort | thermohaline instability and rotation induced mixing in low and intermediate mass stars consequences on global asteroseismic quantities |
url | http://dx.doi.org/10.1051/epjconf/20134301006 |
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