The dark matter halo shape of edge-on disk galaxies: III. Modelling the HI observations: results
This is the third paper in a series in which we attempt to put constraints on the flattening of dark halos in disk galaxies. We observed for this purpose the Hi in edge-on galaxies, where it is in principle possible to measure the force field in the halo
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_O'Brien_The_dark_matter_halo_shape_of_2010.pdf||1.65 MB||Adobe PDF||Request a copy|
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