Discovery of the most isolated globular cluster in the local universe
In Sung Jang, Sungsoon Lim, Hong Soo Park, Myung Gyoon Lee

TL;DR
This paper reports the discovery of the most isolated globular cluster in the local universe, located far from its host galaxies, and characterizes its properties as old, metal-poor, and unusually distant from other known clusters.
Contribution
It presents the identification and detailed analysis of a uniquely isolated globular cluster, expanding understanding of globular cluster distribution and properties.
Findings
GC-2 is the most isolated globular cluster in the local universe.
GC-2 is old (~14 Gyr) and metal-poor ([Fe/H] ≈ -2.3).
GC-2 is located ~400 kpc behind M81, far beyond typical globular clusters.
Abstract
We report the discovery of two new globular clusters in the remote halos of M81 and M82 in the M81 Group based on Hubble Space Telescope archive images. They are brighter than typical globular clusters (MV = -9.34 mag for GC-1 and M_V = -10.51 mag for GC-2), and much larger than known globular clusters with similar luminosity in the MilkyWay Galaxy and M81. Radial surface brightness profiles for GC-1 and GC-2 do not show any features of tidal truncation in the outer part. They are located much farther from both M81 and M82 in the sky, compared with previously known star clusters in these galaxies. Color-magnitude diagrams of resolved stars in each cluster show a well-defined red giant branch (RGB), indicating that they are metal-poor and old. We derive a low metallicity with [Fe/H] and an old age ~14 Gyr for GC-2 from the analysis of the absorption lines in its spectrum in…
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