Model SMC with a NFW profile from equilibrium the movie Watch Video
Preview(s):
Gallery
Play Video: (Note: The default playback of the video is HD VERSION. If your browser is buffering the video slowly, please play the REGULAR MP4 VERSION or Open The Video below for better experience. Thank you!)
Description: This shows the evolution of the dark matter density profile (left) and HI colum density (right) for a model SMC galaxy run with the grid-based astrophysical hydrodynamics code Enzo. The dark matter distribution is run with live dark matter particles, initialized to a NFW profile. The self-gravitating gas is initialized to be in equilibrium with the background dark matter profile. We also embed an initial stellar distribution in the galaxy, represented by a stat background potential. nnThe dark m
Play Video: (Note: The default playback of the video is HD VERSION. If your browser is buffering the video slowly, please play the REGULAR MP4 VERSION or Open The Video below for better experience. Thank you!)