Luminosity-Colour Relations for Red Clump Stars
arXiv:1210.5352 · doi:10.1007/s10509-012-1342-9
Abstract
We calibrated the , , and absolute magnitudes of red clump stars in terms of colours. and are strongly dependent on colour, while the dependence of and on colour is rather weak. The calibration of and absolute magnitudes is tested on 101 RC stars in the field SA 141. The Galactic model parameters estimated with this sample are in good agreement with earlier studies.
12 pages, 14 figures and 4 tables, accepted for publication in Astrophysics and Space Science
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Cited by in corpus (10)
- CCD UBVRI photometry of NGC 6811
- A comprehensive study of the open cluster NGC 6866
- Absolute Magnitudes of Seismic Red Clumps in the Kepler Field and SAGA: the age dependency of the distance scale
- CCD UBV photometry of the open cluster NGC 6819
- Multiwavelength Absolute Magnitudes and Colours of Red Clump Stars in {\it Gaia} Era
- First identification and absolute magnitudes of the red clump stars in the Solar neighbourhood for WISE
- The Chandra Galactic Bulge Survey: optical catalogue and point-source counterparts to X-ray sources
- A New Absolute Magnitude Calibration for Red Clump Stars
- Absolute Magnitude Calibration for Red Clump Stars
- Open cluster age calibration from colour-magnitude morphological indices using Gaia DR3 data