Volume 463, Number 3, March I 2007
|Page(s)||981 - 991|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||19 December 2006|
Early-type stars in the core of the young open cluster Westerlund 2 *,**
Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août, Bât. B5c, 4000 Liège, Belgium e-mail: email@example.com
2 European Southern Observatory, Alonso de Cordova 3107, 19 Vitacura, Santiago, Chile
3 Observatoire de Grenoble, 414 rue de la Piscine, BP 53, 38041 Grenoble, France
4 Département de Physique, Université de Montréal, QC, H3C 3J7, and Observatoire du Mont Mégantic, Canada
Accepted: 3 December 2006
Aims.The properties of the early-type stars in the core of the Westerlund 2 cluster are examined in order to establish a link between the cluster and the very massive Wolf-Rayet binary WR 20a as well as the H ii complex RCW 49.
Methods.Photometric monitoring as well as spectroscopic observations of Westerlund 2 are used to search for light variability and to establish the spectral types of the early-type stars in the cluster core.
Results.The first light curves of the eclipsing binary WR 20a in B and V filters are analysed and a distance of 8 kpc is inferred. Three additional eclipsing binaries, which are probable late O or early B-type cluster members, are discovered, but none of the known early O-type stars in the cluster displays significant photometric variability above 1% at the 1-σ level. The twelve brightest O-type stars are found to have spectral types between O3 and O6.5, significantly earlier than previously thought.
Conclusions.The distance of the early-type stars in Westerlund 2 is established to be in excellent agreement with the distance of WR 20a, indicating that WR 20a actually belongs to the cluster. Our best estimate of the cluster distance thus amounts to kpc. Despite the earlier spectral types, the currently known population of early-type stars in Westerlund 2 does not provide enough ionizing photons to account for the radio emission of the RCW 49 complex. This suggests that there might still exist a number of embedded early O-stars in RCW 49.
Key words: Galaxy: open clusters and associations: individual: Westerlund 2 / stars: early-type / stars: binaries: eclipsing / stars: fundamental parameters / stars: individual: WR 20a
Based on observations collected at the Cerro Tololo Interamerican Observatory and at the European Southern Observatory (La Silla, Chile).
© ESO, 2007
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.