Bibcode
Martín, S.; Alonso, R.; Rodríguez, E.; Ashley, M.; Hidas, M.; Kim, S.-L.; Jeon, Y.-B.; Akan, C.; Poretti, E.; Irwin, M.; de Ugarte, A.; Bossi, M.; Zerbi, F. M.; Suárez, J. C.; Hintz, E. G.
Referencia bibliográfica
In: Second Eddington Workshop: Stellar structure and habitable planet finding, 9 - 11 April 2003, Palermo, Italy. Edited by F. Favata, S. Aigrain and A. Wilson. ESA SP-538, Noordwijk: ESA Publications Division, ISBN 92-9092-848-4, 2004, p. 349 - 353
Fecha de publicación:
1
2004
Número de citas
2
Número de citas referidas
2
Descripción
NGC 6633 is a solar metallicity, young open cluster. In addition to
providing useful information from an asteroseismic point of view, it has
the additional attractiveness of being located in the potential field of
view of the COROT space mission (indeed, it is currently included in the
primary target selection list). We report on some preliminary results
from a multisite photometric monitoring campaign intended to search for
variability in NGC 6633. The detection of δ Scuti stars is a
determining factor in the choice of this open cluster as target of the
COROT Seismology program. We report the detection of new δ Scuti
stars together with other types of pulsating variables (γ Doradus,
SPB, Ap stars, etc.) and some bianry systems.