The Red Giant Branch in the Near-Infrared Colour-Magnitude Diagrams. I: The calibration of photometric indices

Preprint

24 March 2004

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0403563

Abstract

We present new high-quality near-infrared photometry of 10 Galactic Globular Clusters spanning a wide metallicity range (-2.12<[Fe/H]<-0.49): five clusters belong to the Halo (namely, NGC288, NGC362, NGC6752, M15 and M30) and five (namely, NGC6342, NGC6380, NGC6440, NGC6441 and NGC6624) to the Bulge. By combining J, H and K observations with optical data, we constructed Colour-Magnitude Diagrams in various planes (K,J-K), (K,V-K), (H,J-H), and (H,V-H). A set of photometric indices (colours, magnitudes and slopes) describing the location and the morphology of the Red Giant Branch (RGB) have been measured. We have combined this new data set with those already published by Ferraro et al.(2000) and Valenti et al. (2004), and here we present an updated calibration of the various RGB indices in the 2MASS photometric system, in terms of the cluster metallicity.

Keywords

All Related Versions

Version 1, 2004-03-24, ArXiv
Published version: Monthly Notices of the Royal Astronomical Society, 351 (4), 1204.

This publication has 0 references indexed in Scilit: