Volume 478, Number 3, February II 2008
|Page(s)||865 - 868|
|Section||Stellar structure and evolution|
|Published online||12 December 2007|
Photometry of GSC 762-110, a new triple-mode radially pulsating star*
Vereniging Voor Sterrenkunde, Belgium e-mail: email@example.com
2 Zagori Observatory, Epirus, Greece e-mail: firstname.lastname@example.org; email@example.com
3 Helliniki Astronomiki Enosi, Athens, Greece
4 Bundesdeutsche Arbeitsgemeinschaft für Veränderliche Sterne e.V. (BAV), Germany e-mail: firstname.lastname@example.org
5 4030 Linz, Austria e-mail: email@example.com
Accepted: 22 November 2007
Context.Stars pulsating in three radial modes are very rare; only three examples are known in the Galaxy. These stars are very useful since their periods may be measured very precisely, and this will constrain the global stellar parameters and the models of the star's interior.
Aims.The purpose of this paper is to present a new example of the class of triple-mode radial pulsators.
Methods.A search for candidate multi-mode pulsators was carried out in public survey data. Time-series photometry of one of the candidates, GSC 762-110, was performed.
Results.GSC 762-110 was found to be a triple-mode radial pulsator, with a fundamental period of 0.1945 d and period ratios of 0.7641 and 0.8012. In addition two non-radial modes were found, for which the amplitude has diminished considerably over the last few years.
Key words: stars: oscillations / stars: variables: δ Sct / stars: individual: GSC 762-110
© ESO, 2008
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