Shape of dark matter haloes in the Illustris simulation: effects of baryons-Reference-Cited by-同舟云学术

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Shape of dark matter haloes in the Illustris simulation: effects of baryons

Published:2019-01-05 Issue:1 Volume:484 Page:476-493
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Chua Kun Ting Eddie¹²^ORCID,Pillepich Annalisa¹³,Vogelsberger Mark⁴,Hernquist Lars¹

Affiliation:

1. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA

2. Institute of High Performance Computing, 1 Fusionopolis Way, #16-16 Connexis North, Singapore 138632

3. Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany

4. Massachusetts Institute of Technology, Cambridge, MA 02138, USA

Funder

Oak Ridge National Laboratory

Commissariat à l'Énergie Atomique et aux Énergies Alternatives

Singapore National Science Scholarship

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/1/476/27512291/sty3531.pdf

Reference75 articles.

1. Galaxy-induced transformation of dark matter haloes

2. The shape of dark matter haloes: dependence on mass, redshift, radius and formation

3. Internal and External Alignment of the Shapes and Angular Momenta of ΛCDM Halos

4. Transformations of Galaxies. II. Gasdynamics in Merging Disk Galaxies

5. Contraction of dark matter galactic halos due to baryonic infall

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