An asteroseismic study of the β Cephei CoRoT main target HD 180642: results from the ground-based campaign

Bibcode
2009AIPC.1170..394B
DOI
10.1063/1.3246524
Briquet, M.; Uytterhoeven, K.; Morel, T.; Aerts, C.; De Cat, P.; Mathias, P.; Lefever, K.; Miglio, A.; Poretti, E.; Martín-Ruiz, S.; Paparó, M.; Rainer, M.; Carrier, F.; Gutiérrez-Soto, J.; Valtier, J. C.; Benkő, J. M.; Bognár, Zs.; Niemczura, E.; Amado, P. J.; Suárez, J. C.; Moya, A.; Rodríguez-López, C.; Garrido, R.
Referencia bibliográfica

STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference. AIP Conference Proceedings, Volume 1170, pp. 394-396 (2009).

Fecha de publicación:
9
2009
Número de autores
23
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
The β Cephei star HD 180642 was observed by the CoRoT satellite during a run of 156 days in 2007. The space white light photometry revealed the rich frequency spectrum of the star (Degroote et al. 2009). In the present study, we provide additional information on the target, based on both ground-based multi-colour photometry and high-resolution spectroscopy. We place our object in the (Teff, log g) diagram. In addition, we derive the chemical abundances of several elements as well as the metallicity of HD 180642. Finally, we put constraints on the identification of some modes. All these observational constraints will be used to compute stellar models of the target.
Tipo
Sin árbitro

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