Volume 371, Number 1, May III 2001
|Page(s)||107 - 114|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||15 May 2001|
Star clusterings in the Carina complex: photometry of NGC 3324 and Loden 165*
Dipartimento di Astronomia, Universitá di Padova, vicolo dell'Osservatorio 5, 35122 Padova, Italy
2 European Southern Observatory, Karl-Schwartzschild-Str 2, 85748 Garching b. München, Germany
3 Department of Mathematics and Statistics, University of Edinburgh, Edinburgh EH9 3JZ, UK e-mail: firstname.lastname@example.org; email@example.com
Corresponding author: G. Carraro, firstname.lastname@example.org
Accepted: 27 February 2001
We report on UBVRI photometry of two fields in the region of the young open cluster NGC 3324. One of our fields covers the core region, while the other is closer to the tidal radius of the cluster. Our study provides the first CCD photometry of NGC 3324. We find that the cluster is very young and probably contains several pre Main Sequence (MS) stars. 25 members are identified on the basis of their position in the vs. diagram. We investigate the relation of the red super-giant HD 92207 with NGC 3324, suggesting that it probably does not belong to the cluster. Our second field is close to Loden 165, a possible cluster of stars that has never been studied so far. We show that this object is a probable open cluster, much older than NGC 3324 and much closer to the Sun.
Key words: photometry: optical / open clusters and associations: NGC 3324: individual / open clusters and associations: Loden 165: individual
© ESO, 2001
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.