Spectroscopic monitoring of a large samepl of gamma Doradus candidates

Details Spectroscopic monitoring of a large samepl of gamma Doradus candidates Spectroscopic monitoring of a large samepl of gamma Doradus candidates

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..535m&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

Gamma Doradus stars form a new class of variables in between the Sun and the Cepheid Instability Strip, in which gravity modes are currently observed. We present here the first spectroscopic results of an international multisite multitechnique campain concerning These stars with the aim of selecting the best candidate(s) for a proposal for COROT Additional Programs. Indeed, while the COROT core programs concern mainly pressure mode pulsators, gravity-mode stars are interesting because the most internal layers are best probed.

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