Structural and Kinematical Constraints on the Formation of Stellar Nuclear Clusters
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 co...
| Автори: | , , , , |
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| Формат: | Conference item |
| Опубліковано: |
2010
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