Early-type galaxy density profiles from IllustrisTNG – III. Effects on outer kinematic structure
@article{Wang2021EarlytypeGD, title={Early-type galaxy density profiles from IllustrisTNG – III. Effects on outer kinematic structure}, author={Yunchong Wang and Shude Mao and Mark Vogelsberger and Volker Springel and Lars E. Hernquist and Risa H. Wechsler}, journal={Monthly Notices of the Royal Astronomical Society}, year={2021} }
Early-type galaxies (ETGs) possess total density profiles close to isothermal, which can lead to non-Gaussian line-of-sight velocity dispersion (LOSVD) under anisotropic stellar orbits. However, recent observations of local ETGs in the MASSIVE Survey reveal outer kinematic structures at 1.5Reff (effective radius) that are inconsistent with fixed isothermal density profiles; the authors proposed varying density profiles as an explanation. We aim to verify this conjecture and understand the…
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Kinematics of the diffuse intragroup and intracluster light in groups and clusters of galaxies in the local universe within 100 Mpc distance
- PhysicsFrontiers in Astronomy and Space Sciences
- 2022
Nearly all intragroup (IGL) and intracluster light (ICL) comes from stars that are not bound to any single galaxy but were formed in galaxies and later unbound from them. In this review we focus on…
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