The Ubiquity and Dual Nature of Ultra Compact Dwarfs
Mark A. Norris, Sheila J. Kannappan

TL;DR
This paper investigates Ultra Compact Dwarfs (UCDs), revealing two distinct formation channels: some are massive globular clusters, while others are remnants of stripped galaxy nuclei, supported by observational evidence and a unifying formation scheme.
Contribution
It identifies and characterizes two formation pathways for UCDs, integrating them into a unified framework with globular clusters and galaxy nuclei, based on new discoveries and analysis.
Findings
UCDs around NGC3923 are consistent with being giant GCs.
UCD near NGC4546 is a stripped galaxy nucleus with young age.
UCDs above 7x10^7 Msun are almost exclusively stripped nuclei.
Abstract
We present the discovery of several Ultra Compact Dwarfs (UCDs) located in field/group environments. Examination of these objects, plus literature objects, confirms the existence of two distinct formation channels for UCDs. We find that the UCDs we have discovered around the group elliptical NGC3923 (and UCDs generally) have properties consistent with their being the most luminous members of the host galaxy's globular cluster (GC) system. We describe UCDs of this type as giant GCs (GGCs). In contrast, the UCD we have found associated with the isolated S0 NGC4546 is clearly the result of the stripping of a nucleated companion galaxy. The young age (~3.4 Gyr) of the UCD, the lack of a correspondingly young GC population, the apparently short dynamical friction decay timescale (~0.5 Gyr) of the UCD, and the presence of a counterrotating gas disc in the host galaxy (co-rotating with the…
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