other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
2006MNRAS.372..338F - Mon. Not. R. Astron. Soc., 372, 338-342 (2006/October-2)
Complex stellar populations in massive clusters: trapping stars of a dwarf disc galaxy in a newborn stellar supercluster.
FELLHAUER M., KROUPA P. and EVANS N.W.
Abstract (from CDS):
With a set of numerical N-body simulations, we are able to show that, if the mass of the stellar supercluster is high enough and the stellar velocity dispersion in the cluster is comparable to the dispersion of the surrounding disc stars in the host galaxy, then up to about 40 per cent of its initial mass can be additionally gained from trapped disc stars. We also suggest that a supercluster may capture in excess of its own mass under certain conditions.
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): methods: {em N}-body simulations - globular clusters: individual: ω Cen - galaxies: dwarf - galaxies: star clusters
Simbad objects: 6
To bookmark this query, right click on this link: simbad:2006MNRAS.372..338F and select 'bookmark this link' or equivalent in the popup menu