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Thermohaline instability and rotation-induced mixing. III. Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars of various metallicities
Présentation
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Thermohaline instability and rotation-induced mixing. III. Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars of various metallicities
Lagarde, N.
/
Decressin, T.
/
Charbonnel, C.
/
Eggenberger, P.
/
Ekstroem, S.
/
PALACIOS, Ana
- 2012
International audience
Accès au document
Lien externe vers le document:
https://hal.archives-ouvertes.fr/hal-00727306
https://hal.archives-ouvertes.fr/hal-00727306/document
https://hal.archives-ouvertes.fr/hal-00727306/file/aa18331-11.pdf
Métadonnées du document
Auteur(s):
Lagarde, N.
/
Decressin, T.
/
Charbonnel, C.
/
Eggenberger, P.
/
Ekstroem, S.
/
PALACIOS, Ana
- 2012
Editeur:
HAL CCSD
Contributeur:
Université de Genève (UNIGE)
Laboratoire Univers et Particules de Montpellier (LUPM) ; Université Montpellier 2 - Sciences et Techniques (UM2) - IN2P3 - CNRS
Langue:
ANGLAIS
Candidats descripteurs:
instabilities
stars: evolution
stars: interiors
stars: rotation
asteroseismology
[SDU.ASTR.SR] Sciences of the Universe/Astrophysics/Solar and Stellar Astrophysics
[PHYS.ASTR.SR] Physics/Astrophysics/Solar and Stellar Astrophysics
