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20 April 2024
 
  » arxiv » astro-ph/9607081

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CCD photometry of the old open cluster Collinder 261
E. Gozzoli ; M. Tosi ; G. Marconi ; A. Bragaglia ;
Date 16 Jul 1996
Subject astro-ph
AbstractWe present UBVI photometry for the old open cluster Collinder 261. From comparison of the observed colour-magnitude diagrams with simulations based on stellar evolutionary models we derive in a self consistent way reddening, distance, and age of the cluster: E(B-V)=0.25$-$0.34, (m-M)$_0$=11.7-12.0, and age=7$-$8 Gyr or 9$-$11 Gyr, depending on the adopted stellar tracks. The models in better agreement with the data turn out to have metallicity at most solar.
Source arXiv, astro-ph/9607081
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