Physics
Scientific paper
Nov 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..222..171f&link_type=abstract
The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-B
Physics
1
Scientific paper
We present simulation results about the interplay between super star clusters (SSCs) and the host dark-matter (DM) halo, with emphasis on the formation of bulges in very late-type galaxies. Simulations show that the NFW halo close to a stable state has no significant response to sinking of circumnuclear SSCs. Generally speaking, while the halo becomes hotter, its central cusp survives. The structures of the formed bulges are similar to what we obtained with fixed NFW halos, but the bulge formation fraction at various stages are smaller.
Deng Zu-Gang
Fu Yan-Ning
Huang Jia-Hong
No associations
LandOfFree
The role of circumnuclear SSCs in the formation of small bulges does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The role of circumnuclear SSCs in the formation of small bulges, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The role of circumnuclear SSCs in the formation of small bulges will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1112920