Halo mass and assembly history exposed in the faint outskirts: the stellar and dark matter haloes of Illustris galaxies

We use the Illustris simulations to gain insight into the build-up of the outer, low-surface brightness regions which surround galaxies. We characterize the stellar haloes by means of the logarithmic slope of the spherically averaged stellar density profiles, α[subscript STARS] at z = 0, and we rela...

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Bibliographic Details
Main Authors: Pillepich, Annalisa (Author), Vogelsberger, Mark (Contributor), Deason, Alis (Author), Rodriguez-Gomez, Vicente (Author), Genel, Shy (Author), Nelson, Dylan (Author), Torrey, Paul (Author), Sales, Laura V. (Author), Marinacci, Federico (Author), Springel, Volker (Author), Sijacki, Debora (Author), Hernquist, Lars (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: Oxford University Press, 2015-09-10T17:26:10Z.
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