NGC 2587: a sparse open cluster projected onto a populous star field

PIATTI, A.E.; CLARIÁ, J.J.; AHUMADA, A.V.

Rio de Janeiro, Brasil

Simposio; IAU Symposium 266: Star Clusters Basic Galactic Building Blocks throughout Time And Space; 2009

IAU

We present CCD BV IKC photometry in the field of the open cluster NGC 2587. We developed a new method to clean statistically the colour–magnitude diagrams. NGC 2587 is found to be slightly younger than the Hyades and probably of solar metallicity. From 18 probable members with measured proper motions, we derived the following mean cluster values: mu(alpha)=-4.3±3.6 mas/yr and mu(delta)=-2.5±3.4 mas/yr. Colour excesses, E(B-V ) = 0.10 and E(V-I) = 0.15 mag, and a heliocentric distance of 3.7±0.7 kpc are obtained. The interstellar extinction in the cluster direction is found to follow the normal reddening law.