Changes between Version 24 and Version 25 of AstroBearProjects


Ignore:
Timestamp:
06/01/11 18:59:53 (14 years ago)
Author:
Erica Kaminski
Comment:

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  • AstroBearProjects

    v24 v25  
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    2424[[BR]]
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     27'''[BonnerEbert Bonner-Ebert Spheres: Stability, Dynamics, and Collapse] (Erica. [RochesterGroup University of Rochester])'''
     28 * 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.
    2529
    2630'''[ClumpClump/MachStems Bow shock/bow shock Interactions 1: the Formation of Mach Stems] (Kris. [RochesterGroup University of Rochester])'''