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The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks versus Substructures

Debattista, VP, Moore, B, Quinn, T, Kazantzidis, S, Maas, R, Mayer, L, Read, J and Stadel, J (2008) The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks versus Substructures \apj, 681. 1076-1088 - 1076-1088.

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Item Type: Article
Authors :
NameEmailORCID
Debattista, VPUNSPECIFIEDUNSPECIFIED
Moore, BUNSPECIFIEDUNSPECIFIED
Quinn, TUNSPECIFIEDUNSPECIFIED
Kazantzidis, SUNSPECIFIEDUNSPECIFIED
Maas, RUNSPECIFIEDUNSPECIFIED
Mayer, LUNSPECIFIEDUNSPECIFIED
Read, Jj.read@surrey.ac.ukUNSPECIFIED
Stadel, JUNSPECIFIEDUNSPECIFIED
Date : July 2008
Identification Number : 10.1086/587977
Depositing User : Symplectic Elements
Date Deposited : 17 May 2017 12:49
Last Modified : 17 May 2017 15:06
URI: http://epubs.surrey.ac.uk/id/eprint/836839

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