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Non-Perturbative Effect of Rotation on Dipolar Mixed-Modes in Red Giants
Ouazzani, R.-M.; Goupil, M.-J.; Dupret, Marc-Antoine et al.
2013In Astronomical Society of the Pacific Conference Series
 

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Abstract :
[en] The space missions CoRoT (Convection Rotation and Planetary Transits) and Kepler provide high quality data that allows the transport of angular momentum in stars to be investigated by the seismic determination of the internal rotation profile. In a former study (Ouazzani et al. 2013b) we test the validity of seismic diagnostics for red giant rotation that are based on a perturbative method. Our aim here is to investigate oscillation spectra when that validity no longer holds. We use a non-perturbative approach implemented in the Adiabatic Code of Oscillations including Rotation (ACOR code) (Ouazzani et al. 2012) that accounts for the eff
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Ouazzani, R.-M.
Goupil, M.-J.
Dupret, Marc-Antoine ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Marques, J. P.
Lynas-Gray, A. E.
Language :
English
Title :
Non-Perturbative Effect of Rotation on Dipolar Mixed-Modes in Red Giants
Publication date :
01 December 2013
Event name :
Progress in Physics of the Sun and Stars: A New Era in Helio- and Asteroseismology.
Event date :
25-29 Novembre 2012
Audience :
International
Main work title :
Astronomical Society of the Pacific Conference Series
Pages :
335
Commentary :
479
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since 12 February 2014

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