期刊
ASTRONOMY & ASTROPHYSICS
卷 499, 期 3, 页码 967-982出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/200911691
关键词
stars: variables: general; stars: oscillations; stars: individual: gamma Doradus; techniques: photometric
资金
- Fund for Scientific Research-Flanders (FWO) [G.0178.02, G.0332.06]
- Research Council of K.U. Leuven [GOA/2008/04]
- European Research Council [FP7/2007-2013, 227224]
Context. gamma Dor stars are excellent targets for asteroseismology since the gravity modes present in these stars probe the deep stellar interiors. Mode identification will improve the knowledge of these stars considerably. Aims. A selected group of gamma Dor stars and some candidates were observed with the Mercator telescope to find and/or confirm the periodicities in the light variations and to derive reliable amplitude ratios in different pass bands. Methods. A frequency analysis was performed on all new data obtained in the Geneva photometric system. In order to have more reliable and accurate frequencies, the new data were combined with similar data from the literature and with Hipparcos observations. A set of frequencies that minimized the residuals in a harmonic fit was searched for while allowing means and amplitudes to vary from one observation set to another. Results. Frequencies and amplitudes in the photometric passbands of the Geneva system are given for 21 gamma Dor stars. We report the discovery of HD 74504 as a newly found gamma Dor star. Conclusions. Our study provides the first extensive multicolour database for the understanding of gravity modes in F-type stars.
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