Volume 411, Number 2, November IV 2003
|Page(s)||83 - 90|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||17 November 2003|
Discovery of new Milky Way star cluster candidates in the 2MASS Point Source Catalog. II. Physical properties of the star cluster CC 01*
Pontificia Universidad Católica de Chile, Facultad de Física, Departamento de Astronomía y Astrofísica, Av. Vicuña Mackenna 4860, 782-0436 Macul, Santiago, Chile
2 Department of Astronomy, Sofia University, Bulgaria, and Isaac Newton Institute of Chile, Bulgarian Branch, 5 James Bourchier, 1164 Sofia, Bulgaria e-mail: [pessev, kurtev, givanov]@phys.uni-sofia.bg
3 European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei Mnchen, Germany e-mail: firstname.lastname@example.org
4 European Southern Observatory, Ave. Alonso de Cordova 3107, Casilla 19, Santiago 19001, Chile e-mail: email@example.com
Corresponding author: J. Borissova, firstname.lastname@example.org
Accepted: 21 August 2003
Three new obscured Milky Way clusters were detected as surface density peaks in the 2MASS point source catalog during our on-going search for hidden globular clusters and massive Arches-like star clusters. One more cluster was discovered serendipitously during a visual inspection of the candidates. The first deep J, H, and Ks imaging of the cluster [IBP 2002] CC 01 is presented. We estimated a cluster age of ~1–3 Myr, distance modulus of mag ( kpc), and extinction of mag. We also derived the initial mass function slope for the cluster: ). The integration over the initial mass function yielded a total cluster mass . CC 01 appears to be a regular, not very massive star cluster, whose formation has probably been induced by the shock front from the nearby Hii region Sh 2-228.
Key words: Galaxy: open clusters and associations: general / infrared: general
© ESO, 2003
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