Volume 396, Number 1, December II 2002
|Page(s)||125 - 130|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||22 November 2002|
Proper motions and CCD-photometry of stars in the region of the open cluster NGC 1513*
The Main Astronomical Observatory, Pulkovo, St. Petersburg, Russia
2 Laboratório Nacional de Computação Científica / MCT, Petrópolis, RJ, Brazil
Corresponding author: V. N. Frolov, The Main Astronomical Observatory, Pulkovo, St. Petersburg, Russia firstname.lastname@example.org
Accepted: 10 September 2002
The results of astrometric and photometric investigations of the poorly studied open cluster NGC 1513 are presented. The proper motions of 333 stars with a root-mean-square error of were obtained by means of the automated measuring complex “Fantasy”. Eight astrometric plates covering the time interval of 101 years were measured and a total of 141 astrometric cluster members identified. BV CCD-photometry was obtained for stars in an area centered on the cluster. Altogether 33 stars were considered to be cluster members with high reliability by two criteria. The estimated age of NGC 1513 is years.
Key words: open clusters and associations: general / open clusters and associations: individual: NGC 1513
© ESO, 2002
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