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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. GroenewegenInstituut 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
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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