The globular cluster system of an ``old'' merger: NGC 5018
| dc.creator | Hilker, Michael | |
| dc.creator | Kissler-Patig, Markus | |
| dc.date | 1996-05-09 | |
| dc.date.accessioned | 2026-07-07T02:21:15Z | |
| dc.date.available | 2026-07-07T02:21:15Z | |
| dc.description | 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). (...) | |
| dc.description | Accepted for publication in A&A. 12 pages, gzipped, uuencoded, including 9 figures. Also available at http://aibn55.astro.uni-bonn.de:8000/~mkissler/ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9605040 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9605040 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/10479 | |
| dc.subject | Astrophysics | |
| dc.title | The globular cluster system of an ``old'' merger: NGC 5018 | |
| dc.type | text |