On the Kinematics, Stability and Lifetime of Kinematically Distinct Cores: A Case Study
We present a case study of a early-type galaxy (ETG) hosting a kinematically distinct core (KDC) formed in a binary high resolution 1:1 spiral galaxy merger simulation. The runtime of the simulation is pushed up to 10 Gyr to follow the complete evolution of various physical properties. To i...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2017-08-01
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Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/5/3/41 |