Investigating Dark Matter Profiles of Core Galaxies
Li-Chin Yeh2, Ing-Guey Jiang1*
1Institute of Astronomy, National Tsing Hua University, Hsin-Chu, Taiwan
2Institute of Computational and Modeling Sciences, National Tsing Hua University, Hsin-Chu, Taiwan
* Presenter:Ing-Guey Jiang,
Core galaxies are those early-type galaxies with flat central surface brightness.
It is still unclear how they could form given that the central mass density distributions of galaxies are predicted to have cusp profiles . The core galaxy NGC 1399 is modeled through a particle-based method here. The dark matter profile, and the existence of single or binary supermassive black holes are investigated. The possible formation scenario of core galaxies will also be addressed.

Keywords: galaxies, supermassive black holes, dark matter