Volume 385, Number 2, April II 2002
|Page(s)||471 - 478|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||15 April 2002|
The cases of NGC 7036 and NGC 7772
Dipartimento di Astronomia, Università di Padova, Vicolo Osservatorio 2, 35122 Padova, Italy
Corresponding author: firstname.lastname@example.org
Accepted: 17 January 2002
We present CCD UBVI observations obtained in the field of the two previously unstudied dissolving open cluster candidates NGC 7036 and NGC 7772. Our analysis suggests that both the objects are Open Cluster Remnants (OCR). NGC 7036 is an open cluster remnant with a core radius of about 3–4 arcmin. We derive for the first time estimates of its fundamental parameters. We identify 17 likely members that define a group of stars at 1 kpc from the Sun, with a low reddening , and with an age of about 3–4 Gyr. As for NGC 7772, we identify 14 likely members, that define a group of stars with a very low reddening (), are 1.5 Gyr old and are located about 1.5 kpc from the Sun.
Key words: open clusters and associations: individual: NGC 7036, NGC 7772 - 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.