An extended star formation history in an ultra-compact dwarf

There has been significant controversy over the mechanisms responsible for forming compact stellar systems like ultra-compact dwarfs (UCDs), with suggestions that UCDs are simply the high-mass extension of the globular cluster population, or alternatively, the liberated nuclei of galaxies tidally st...

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Bibliographic Details
Published in:	Monthly notices of the Royal Astronomical Society 2015-08, Vol.451 (4), p.3615-3626
Main Authors:	Norris, Mark A, Escudero, Carlos G, Faifer, Favio R, Kannappan, Sheila J, Forte, Juan Carlos, van den Bosch, Remco C. E
Format:	Article
Language:	eng
Subjects:	Dispersions Dwarf stars Galaxies Kinematics Nuclei Signal to noise ratio Star & galaxy formation Star formation Stellar systems
Online Access:	Get full text
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Summary:	There has been significant controversy over the mechanisms responsible for forming compact stellar systems like ultra-compact dwarfs (UCDs), with suggestions that UCDs are simply the high-mass extension of the globular cluster population, or alternatively, the liberated nuclei of galaxies tidally stripped by larger companions. Definitive examples of UCDs formed by either route have been difficult to find, with only a handful of persuasive examples of stripped-nucleus-type UCDs being known. In this paper, we present very deep Gemini/GMOS spectroscopic observations of the suspected stripped-nucleus UCD NGC 4546-UCD1 taken in good seeing conditions (
ISSN:	0035-8711 1365-2966