Structural and Kinematical Constraints on the Formation of Stellar Nuclear Clusters

Details Structural and Kinematical Constraints on the Formation of Stellar Nuclear Clusters Structural and Kinematical Constraints on the Formation of Stellar Nuclear Clusters

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1240..243h&link_type=abstract

HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. Edited by Victor P. Debattista and Cristina C. Popescu AIP Conferen

Computer Science

Star Formation, Spiral Galaxies, Accretion, Merging, Star Formation, Spiral Galaxies, Infall, Accretion, And Accretion Disks, Galaxy Mergers, Collisions, And Tidal Interactions

Scientific paper

We study the formation of stellar nuclear clusters (NC) with two types of N-body simulations: mergers of star clusters (SC) at the centre of disk galaxies and the accretion of a SC onto a previous NC. The merging of SCs produces systems consistent with observed scaling relations, they have shapes comparable with those observed and rotation consistent with that observed in the NCs of NGC 4244 and M 33.

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