Reference : A procedure for modelling asymptotic g-mode pulsators: The case of gamma Doradus stars
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/76463
A procedure for modelling asymptotic g-mode pulsators: The case of gamma Doradus stars
English
Moya, A. [Instituto de Astrofísica de Andalucía -CSIC, Cno. Bajo de Huetor, 18008, Granada, Spain]
Suárez, J. C. [Instituto de Astrofísica de Andalucía -CSIC, Cno. Bajo de Huetor, 18008, Granada, Spain]
Martín-Ruiz, S. [Instituto de Astrofísica de Andalucía -CSIC, Cno. Bajo de Huetor, 18008, Granada, Spain]
Amado, P. J. [Instituto de Astrofísica de Andalucía -CSIC, Cno. Bajo de Huetor, 18008, Granada, Spain]
Rodríguez-López, C. [Instituto de Astrofísica de Andalucía -CSIC, Cno. Bajo de Huetor, 18008, Granada, Spain]
Grigahcène, A. [CRAAG, Algiers Observatory, BP 63 Bouzareah 16340, Algiers, Algeria]
Dupret, Marc-Antoine [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique >]
Rodríguez, E. [Instituto de Astrofísica de Andalucía -CSIC, Cno. Bajo de Huetor, 18008, Granada, Spain]
Garrido, R. [Instituto de Astrofísica de Andalucía -CSIC, Cno. Bajo de Huetor, 18008, Granada, Spain]
2008
Astronomische Nachrichten
329
541
Yes (verified by ORBi)
International
0004-6337
[en] stars: evolution ; stars: interiors ; stars: oscillations ; stars: rotation ; stars: fundamental parameters
[en] Mode identification is one of the first and main problems we encounter in trying to develop the complete potential of asteroseismology. In the particular case of {g}-mode pulsators, this is still an unsolved problem, from both the observational and theoretical points of view. Nevertheless, in recent years, some observational and theoretical efforts have been made to find a solution. In this work we use the latest theoretical and computational tools to understand asymptotic {g}-mode pulsators: 1) the Frequency Ratio Method, and 2) Time Dependent Convection. With these tools, a self-consistent procedure for mode identification and modelling of these {g}-mode pulsators can be constructed. This procedure is illustrated using observational information available for the gamma Doradus star 9 Aurigae.
http://hdl.handle.net/2268/76463
10.1002/asna.200710993
http://adsabs.harvard.edu/abs/2008AN....329..541M

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