Near Infrared properties of 12 Globular Clusters toward the inner Bulge of the Galaxy

E. Valenti; F. R. Ferraro; L. Origlia

doi:10.1111/j.1365-2966.2009.15991.x

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arXiv · 0911.1264

Near Infrared properties of 12 Globular Clusters toward the inner Bulge of the Galaxy

E. Valenti·F. R. Ferraro·L. Origlia

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Abstract

We present near-IR Colour-Magnitude diagrams and physical parameters for a sample of 12 galactic globular clusters located toward the inner Bulge region. For each cluster we provide measurements of the reddening, distance, photometric metallicity, luminosity of the horizontal branch red clump, and of the red giant branch bump and tip. The sample discussed here together with that presented in Valenti, Ferraro & Origlia (2007) represent the largest homogeneous catalog of Bulge globular clusters (comprising ~ 80% of the entire Bulge cluster population) ever studied. The compilation is available in electronic form on the World Wide Web (http://www.bo.astro.it/~GC/ir_archive)

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E. Valenti, F. R. Ferraro, L. Origlia. 2009-11-06. Near Infrared properties of 12 Globular Clusters toward the inner Bulge of the Galaxy. https://doi.org/10.1111/j.1365-2966.2009.15991.x

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