Testing the identification of p-mode frequencies in solar-like stars

Bibcode
2004ESASP.538..393R
Régulo, C.; Pérez Hernández, F.; Roca-Cortés, T.
Referencia bibliográfica

In: Second Eddington Workshop: Stellar structure and habitable planet finding, 9 - 11 April 2003, Palermo, Italy. Edited by F. Favata, S. Aigrain and A. Wilson. ESA SP-538, Noordwijk: ESA Publications Division, ISBN 92-9092-848-4, 2004, p. 393 - 396

Fecha de publicación:
1
2004
Número de autores
3
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
1
Descripción
The regular pattern that high n p-mode frequencies of solar-like stars show is used to design a method for a quick check to the identification of the modes. The case of a wrong mode identification or a spurious one is clearly shown by the method, which depends rather weakly on the possible stellar models. An application of the method shows evidences of misidentification in the recent frequencies of α Cen A suggested by Bouchy & Carrier (2002).
Tipo
Sin árbitro
Métodos

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