Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-11-04
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
To be published in Astrophysics and Space Science Proceedings series (ASSP), in the proceedings of "20th Stellar Pulsation Con
Scientific paper
The study of open clusters and their short period variable stars is fundamental in stellar evolution. Because the cluster members are formed in almost the same physical conditions, they share similar stellar properties such age and chemical composition. The assumption of common age, metallicity and distance impose strong constraints when modeling an ensemble of short period pulsators belonging to open clusters (e.g. Fox Machado et al., 2006). Very recently, Luo et al. (2009) carried out a search for variable stars in the direction of NGC 6811 with CCD photometry in B and V bands. They detected a total of sixteen variable stars. Among these variables, twelve were catalogued as $\delta$ {\it Scuti} stars, while no variability type was assigned to the remaining stars. In this paper we present $uvby\beta$ photoelectric photometry for the variable stars in the direction of NGC 6811.
Espinosa Allan
Fox-Machado Lester
García Hector
Peña José H.
Rentería Alejandro
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