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arXiv · astro-ph/9605040

The globular cluster system of an ``old'' merger: NGC 5018

Michael Hilker·Markus Kissler-Patig
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Abstract

We study the properties of the globular cluster system of the ``old'' merger NGC 5018. We detect a relatively poor globular cluster system, that can be divided into at least two populations based on colors: a small population of blue clusters, aged between several hundred Myr to 6 Gyr, the formation of which was probably induced by the last interaction in the galaxy group; and one (possibly two) population(s) of old(er) clusters that can be associated with the original galaxy(ies). (...)

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Michael Hilker, Markus Kissler-Patig. 1996-05-09. The globular cluster system of an ``old'' merger: NGC 5018. https://arxiv.org/abs/astro-ph/9605040

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