An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy. Large separation as a new observable for δ Scuti stars

A. García Hernández , A. Moya (1) , E. Michel (2) , J. Suárez , E. Poretti (3) , S. Martín-Ruíz , P. Amado , R. Garrido (4) , E. Rodríguez (4) , M. Rainer , K. Uytterhoeven (5) , C. Rodrigo (6) , E. Solano (7) , J. Rodon (8) , P. Mathias (9) , A. Rolland , M. Auvergne (2) , A. Baglin (2) , F. Baudin (10) , C. Catala (2) , R. Samadi (2)

1 ICBiBE - Institut Cavanilles de Biodiversitat i Biologia Evolutiva
2 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
3 OAB - INAF - Osservatorio Astronomico di Brera
4 IAA - Instituto de Astrofísica de Andalucía
5 IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers
6 Instituto IMDEA Nanociencia [Madrid]
7 SVO - Spanish Virtual Observatory - Observatorio Virtual Español
8 LAM - Laboratoire d'Astrophysique de Marseille
9 FIZEAU - Laboratoire Hippolyte Fizeau
10 IAS - Institut d'astrophysique spatiale

Domaines: Physique [physics]; Astrophysique [astro-ph]

A. García Hernández, A. Moya, E. Michel, J. Suárez, E. Poretti, et al.. An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy. Large separation as a new observable for δ Scuti stars. Astronomy and Astrophysics - A&A, 2013, 559, pp.A63. ⟨10.1051/0004-6361/201220256⟩. ⟨hal-02551795⟩