An Ongoing Tidal Capture in the Large Magellanic Cloud: The Low-mass Star Cluster KMK 88-10 Captured by the Massive Globular Cluster NGC 1835?*

In the context of a project aimed at characterizing the dynamical evolution of old globular clusters in the Large Magellanic Cloud, we have secured deep HST/WFC3 images of the massive cluster NGC 1835. In the field of view of the acquired images, at a projected angular separation of approximately 2 & PRIME; from the cluster, we detected the small stellar system KMK 88-10. The observations provided the deepest color-magnitude diagram ever obtained for this cluster, revealing that it hosts a young stellar population with an age of 600-1000 Myr. The cluster surface brightness profile is nicely reproduced by a King model with a core radius r ( c ) = 4 & DPRIME; (0.97 pc), a half-mass radius r ( hm ) = 12 & DPRIME; (2.9 pc), and a concentration parameter c & SIM; 1.3 corresponding to a truncation radius r ( t ) & SIM; 81 & DPRIME; (19.5 pc). We also derived its integrated absolute magnitude (M ( V ) = -0.71) and total mass (M & SIM; 80-160 M (& ODOT;)). The most intriguing feature emerging from this analysis is that KMK 88-10 presents a structure elongated in the direction of NGC 1835, with an intracluster overdensity that suggests the presence of a tidal bridge between the two systems. If confirmed, this would be the first evidence of a tidal capture of a small star cluster by a massive globular.