Volume 401, Number 3, April III 2003
|Page(s)||1077 - 1086|
|Section||Stellar structure and evolution|
|Published online||01 April 2003|
Evidence of the γ Doradus nature for a group of candidates
INAF-Osservatorio Astronomico di Brera, via Bianchi 46, 23807 Merate (LC), Italy e-mail: firstname.lastname@example.org; email@example.com
Corresponding author: S. Martín, firstname.lastname@example.org
Accepted: 31 January 2003
We present in this paper new photometry of eight stars suspected to be γ Doradus variables according to Handler & Kaye (2000). The new observational material has been analyzed and previously published data re-analyzed by means of an objective period search technique, based on the least-squares algorithm, called Multifre (Bossi & Nuñez 2002). We found evidence for the inclusion of seven of these stars in the list of recognized γ Doradus variables.
Key words: stars: variables: general / stars: oscillations / stars: fundamental parameters / techniques: photometric
© ESO, 2003
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