Proper Motions and CCD-photometry of Stars in the Region of the Open Cluster NGC 1513

2); (2) LNCC / MCT; Btazil); D.L. Gorshanov (1). ((1)The Main Astronomical Observatory; E.G. Jilinski (1; E.V. Poljakov (1); J.K. Ananjevskaja (1); N.M. Bronnikova (1); Petropolis; Pulkovo

arxiv: astro-ph/0212255 · v1 · submitted 2002-12-11 · 🌌 astro-ph

Proper Motions and CCD-photometry of Stars in the Region of the Open Cluster NGC 1513

V.N. Frolov (1) , E.G. Jilinski (1 , 2) , J.K. Ananjevskaja (1) , E.V. Poljakov (1) , N.M. Bronnikova (1) , D.L. Gorshanov (1). ((1)The Main Astronomical Observatory , Pulkovo

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St. Petersburg Russia (2) LNCC / MCT Petropolis RJ Btazil)

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keywords clusterstarsastrometricarcminccd-photometrymembersmotionsopen

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The results of astrometric and photometric investigations of the poorly studied open cluster NGC 1513 are presented. The proper motions of 353 stars with the root-mean-square error of 1.9 mas/yr were obtained by means of the automated measuring complex "Fantasy" scanning of 8 astrometric plates covering the time interval of 101 years. A total of 141 astrometric cluster members have been identified. BV CCD-photometry was made for the stars in a square size 17 arcmin x 17 arcmin centered on cluster. 33 stars with the high reliability were considered to be cluster members by two criteria. The estimation of NGC 1513 age is 2.54 E+08 years. Tables 2 and 3 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/.

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Proper Motions and CCD-photometry of Stars in the Region of the Open Cluster NGC 1513

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