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Astron. Astrophys. Suppl. Ser.
Volume 133, Number 1, November_II 1998
Page(s) 25 - 28
Published online 15 November 1998
DOI: 10.1051/aas:1998453

Astron. Astrophys. Suppl. Ser. 133, 25-28

CCD photometry of distant open clusters

IV. Trumpler 5[*]

J. Kaluzny

Send offprint request: J. Kaluzny

Warsaw University Observatory, Al. Ujazdowskie  4, 00-478 Warsaw, Poland

Received April 21; accepted May 13, 1998


We present BVI photometry for Trumpler 5, a rich open cluster located in the Galactic anticenter. The cluster age is slightly lower than the age of M 67. Its distance modulus (m-M)0 and reddening E(B-V) are estimated at 12.4 and 0.58, respectively. These values were obtained for the assumed solar metallicity of the cluster. Our data indicate that Tr 5 is one of the richest objects among the sample of known old open clusters. The total mass included only in upper-main sequence stars exceeds 3000 $m_{\odot}$. The angular diameter of the cluster is estimated at 11.6 arcmin, which corresponds to a linear size of about 20 pc for an estimated distance $d\approx 3.0$ kpc[*].

Key words: open clusters and associations: individual: Trumpler 5 -- HR diagram

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