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arXiv · 0710.2030

FSR0190 - Another old distant galactic cluster

D. Froebrich·H. Meusinger·C. J. Davis
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Abstract

We are conducting a large program to classify newly discovered Milky Way star cluster candidates from Froebrich et al. (2007). Here we present NIR follow-up observations of FSR0190 (RA=20h05m31.3s, DEC=33deg34'09" J2000). The cluster is situated close to the Galactic Plane (l=70.7302deg, b=+0.9498deg). It shows a circular shape, a relatively large number of core helium burning stars -- which clearly distinguishes the cluster from the rich field -- but no centrally condensed star density profile. We derive an age of more than 7Gyr, a Galactocentric distance of 10.5kpc, a distance of 10kpc from the Sun, and an extinction of A_K=0.8mag. The estimated mass is at least of the order of 1E5M_sun, and the absolute brightness is M_V<=-4.7mag; both are rather typical properties for Palomar-type globular clusters.

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D. Froebrich, H. Meusinger, C. J. Davis. 2007-10-10. FSR0190 - Another old distant galactic cluster. https://doi.org/10.1111/j.1745-3933.2007.00409.x

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