- Levine et al.
- http://arxiv.org/abs/0711.3478
- Simulation with high dynamic range (1E7) down to 0.1pc, i.e. to the accretion disk of a SMBH.
- Global instabilities make things quasi-stable locally due to turbulence.
- An exponential density profile for the gas in a disk arises naturally due to this.
You are currently browsing articles tagged Disk.
Tags: Black Holes, Disk, Galaxies, Simulation
- Lee at al.
- http://arxiv.org/abs/0711.1232
- The GCs around Andromeda rotate.
- GCs can be “friendless”, meaning they have no neighbors with similar kinematics. In addition they look at various subsamples depending e.g. on metallicity and brightness.
Tags: Disk, Galaxies, GC, Kinematics