The globular cluster AM 4: yet another young globular associated with the Sgr Dwarf Spheroidal galaxy?

The complete census of globular clusters formerly belonging to the Sgr dSph and now deposited into the Galactic halo is an important contribution to our comprehension of the evolution and disruption of this dwarf galaxy. We investigate in this study the possibility that the poorly known “old” globular AM 4 might be associated with the Sagittarius dwarf galaxy, and at the same time provide more solid estimate of its basic parameters. New high quality BVI photometry is presented, from which an improved Color Ma gnitude Diagram is constructed, and estimates of age and distance are then derived. The distance and Galactic position are finally investigated in details. AM4 is found to be a low luminosity (M$_V$=-1.82) cluster undergoing strong tidal stress by the Milky Way and on the verge to be dissolved. Besides, and at odds with previous suggestions, we provide evidences that AM 4 is indeed young, with an age around 9 Gyrs (as Terzan7), but somewhat more metal poor ([Fe/H=-0.97]). AM~4 is located at 33$_{-4}^{+3}$ kpc from the Sun, in a direction and at distance not totally incompatible with the Sgr dSph stream. Although we significantly improved our knowledge of AM 4, further studies are encouraged to obtain radial velocity and metallicity to d emonstrate more firmly (or deny) the association to Sgr

💡 Research Summary

The paper addresses the long‑standing question of whether the faint Milky Way globular cluster AM 4 originated in the Sagittarius dwarf spheroidal galaxy (Sgr dSph) and, in the process, provides a substantially improved set of fundamental parameters for the cluster. Using newly obtained deep B, V, and I imaging, the authors construct a high‑quality color‑magnitude diagram (CMD) that reveals a clear main‑sequence turn‑off and red‑giant branch. Isochrone fitting to the CMD yields an age of roughly 9 ± 1 Gyr, a metallicity of