arXiv:1210.5352 [astro-ph.GA]AbstractReferencesReviewsResources
Luminosity-Colour Relations for Red Clump Stars
S. Bilir, O. Onal, S. Karaali, A. Cabrera-Lavers, H. Cakmak
Published 2012-10-19, updated 2012-10-27Version 2
We calibrated the $M_V$, $M_J$, $M_{K_s}$ and $M_g$ absolute magnitudes of red clump stars in terms of colours. $M_V$ and $M_g$ are strongly dependent on colour, while the dependence of $M_J$ and $M_{K_s}$ on colour is rather weak. The calibration of $M_V$ and $M_{K_s}$ 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.
Comments: 12 pages, 14 figures and 4 tables, accepted for publication in Astrophysics and Space Science
Categories: astro-ph.GA
Tags: journal article
Related articles: Most relevant | Search more
arXiv:1304.0435 [astro-ph.GA] (Published 2013-04-01)
First identification and absolute magnitudes of the red clump stars in the Solar neighbourhood for WISE
On the Age Calibration of Open Clusters using Red Clump Stars
arXiv:1905.11944 [astro-ph.GA] (Published 2019-05-28)
Mapping the Galactic disk with red clump stars from LAMOST and Gaia II: 3D asymmetrical kinematics of mono-age populations in the disk between 6-14 kpc
H. -F. Wang et al.