Volume 387, Number 2, May IV 2002
|Page(s)||479 - 486|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||13 May 2002|
Dipartimento di Astronomia, Università di Padova, Vicolo Osservatorio 2, 35122 Padova, Italy
Corresponding author: firstname.lastname@example.org
Accepted: 5 March 2002
We present CCD UBVI observations obtained in the field of the previously unstudied northern open clusters NGC 133 and NGC 1348. We argue that NGC 133 is a heavily contaminated cluster, for which we identify 13 candidate members down to mag on the basis of the position in the two-color Diagram. Membership has been checked against proper motions from Tycho 2, whenever available. The cluster turns out to have a reddening mag, to be pc distant from the Sun, and to have an age less than 10 Myrs. NGC 1348 is a more reddened clusters ( mag) for which we isolate 20 members. The cluster lies at a distance of kpc away from the Sun, and has an age greater than 50 Myrs.
Key words: open clusters and associations: individual: NGC 133, NGC 1348 – open clusters and associations: general
© ESO, 2002
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.