Changes between Version 28 and Version 29 of AstroBearProjects

Timestamp:

06/10/11 17:58:24 (14 years ago)

Author:

kris

Comment:

Added LANL, moved up Christina's project

AstroBearProjects

@@ -16 +16 @@
    * Computing systems TBA
 
+  * [LanlGroup Los Alamos National Lab]
+
 [[BR]]
 
@@ -29 +31 @@
 '''[BonnerEbert Bonner-Ebert Spheres: Stability, Dynamics, and Collapse] (Erica. [RochesterGroup University of Rochester])'''
  * Stars form from the collapse of self-gravitating clouds. These clouds can be modelled by Bonner-Ebert spheres, which are isothermal spheres in hydrostatic equilibrium. This numerical study aims to explore the stability of Bonner-Ebert spheres, their dynamics (i.e. rotation, MHD effects, turbulence), and the subset of conditions in which collapse is triggered in relation to star formation theory.
+
+'''Supersonic colliding clouds and star formation (Christina. [NorthCarolinaGroup University of North Carolina, Chapel Hill])'''
+ * Studying star formation at the edge of colliding flows in large cloud formations.  Exploring the effects of NTSI, thermal instability, and shear flows on star formation rates in these regions.
+ * [wiki:Clouds Module Explanation]
 
 '''[ClumpClump/MachStems Bow shock/bow shock Interactions 1: the Formation of Mach Stems] (Kris. [RochesterGroup University of Rochester])'''
@@ -75 +81 @@
 
 
-'''Supersonic colliding clouds and star formation (Christina. [NorthCarolinaGroup University of North Carolina, Chapel Hill])'''
- * Studying star formation at the edge of colliding flows in large cloud formations.  Exploring the effects of NTSI, thermal instability, and shear flows on star formation rates in these regions.
- * [wiki:Clouds Module Explanation]