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

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

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

Advertised on:
1
2004
Number of authors
3
IAC number of authors
0
Citations
1
Refereed citations
1
Description
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).
Type
Non-refereed
Methods

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