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Issue A&A
Volume 463, Number 2, February IV 2007
Page(s) 559 - 565
Section Galactic structure, stellar clusters, and populations
DOI http://dx.doi.org/10.1051/0004-6361:20052721



A&A 463, 559-565 (2007)
DOI: 10.1051/0004-6361:20052721

K-band magnitude of the red clump as a distance indicator

V. Van Helshoecht and M. A. T. Groenewegen

Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
    e-mail: veerle@ster.kuleuven.be

(Received 18 January 2005 / Accepted 21 September 2006)

Abstract
We have investigated how the K-band magnitude of the red clump [MK(RC)] depends on age and metallicity, using 2MASS infrared data for a sample of 24 open clusters with known distances. We show that a constant value of $M_K(RC)=-1.57 \pm 0.05$ is a reasonable assumption to use in distance determinations for clusters with metallicity between -0.5 and +0.4 dex and age between 108.5 and 109.9 years.


Key words: open clusters and associations: general -- stars: horizontal-branch -- stars: distances



© ESO 2007


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