Low Surface Brighness galaxies: Vc-s0 relation and halo central density radial profile from stellar kinematics measurements
Sissa Medialab Srl (2004) 046
The Cosmological Context of Extraplanar Gas
ArXiv astro-ph/0409639 (2004)
Abstract:
I review evidence that galaxies form from gas that falls into potential wells cold, rather than from virialized gas, and that formation stops once an atmosphere of trapped virialized gas has accumulated. Disk galaxies do not have such atmospheres, so their formation is ongoing. During galaxy formation feedback is an efficient process, and the nuclear regions of disk galaxies blow winds. The cold infalling gas that drives continued star formation has a significant component of angular momentum perpendicular to that of the disk. Extraplanar gas has to be understood in the context set by nuclear outflows and cold skew-rotating cosmic infall.Can Virialization Shocks be Detected Around Galaxy Clusters Through the Sunyaev-Zel'dovich Effect?
(2004)
Evolution of self-gravitating magnetized disks. II- Interaction between MHD turbulence and gravitational instabilities
(2004)
Mapping stationary axisymmetric phase-space distribution functions by orbit libraries
Monthly Notices of the Royal Astronomical Society 353:2 (2004) 391-404