Halo expansion in cosmological hydro simulations: toward a baryonic solution of the cusp/core problem in massive spirals

Find Full text

Files in this item


Copyright statement:

Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
Published Version: http://dx.doi.org/10.1088/2041-8205/744/1/L9

This item appears in the following Collection(s)

Search DSpace


My Account