The Cycle of Gaseous Baryons Between the Disk and Halo
The gaseous halo surrounding a galaxy disk is often referred to as the circum-galactic medium (CGM). The boundary of the CGM is loosely defined as the virial radius of the galaxy. Recent observations and simulations have shown that the CGM is massive, multiphase, clumpy, and metal-enriched. The CGM...
Main Author: | Zheng, Yong |
---|---|
Language: | English |
Published: |
2018
|
Subjects: | |
Online Access: | https://doi.org/10.7916/D8K661M4 |
Similar Items
-
The structure of dark matter halos and disk galaxy rotation curves
by: Hayashi, Eric Jeffrey.
Published: (2008) -
The evolution of disk galaxies in cold dark matter halos
by: Font, Andreea S.
Published: (2008) -
Inferring the 3D gravitational field of the Milky Way with stellar streams
by: Price-Whelan, Adrian Michael
Published: (2016) -
Dark Matter Halos: Assembly, Clustering and Sub-halo Accretion
by: Li, Yun
Published: (2010) -
Investigating the Andromeda stream : a simple analytic bulge-disk-halo model for M31
by: Geehan, Jonathan James
Published: (2008)