Projected alignment of non-sphericities of stellar, gas, and dark matter distributions in galaxy clusters: analysis of the Horizon-AGN simulation

Author:

Okabe Taizo1,Nishimichi Takahiro2,Oguri Masamune123,Peirani Sébastien145,Kitayama Tetsu6,Sasaki Shin7,Suto Yasushi13

Affiliation:

1. Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

2. Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583, Japan

3. Research Center for the Early Universe, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan

4. Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’ Observatoire, Université Côte d’Azur, CS 34229, F-06304 Nice Cedex 4, France

5. Institut d’Astrophysique de Paris (UMR 7095: CNRS and UPMC), 98 bis Bd Arago, F-75014 Paris, France

6. Department of Physics, Toho University, Funabashi, 2-2-1 Miyama, Funabashi, Chiba 274-8510, Japan

7. Department of Physics, Tokyo Metropolitan University, 1-1 Minami-Osawa, Hachioji, Tokyo 192-0397, Japan

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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