Radiation hydrodynamics simulations of the formation of direct-collapse supermassive stellar systems-Reference-Cited by-同舟云学术

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Radiation hydrodynamics simulations of the formation of direct-collapse supermassive stellar systems

Published:2018-01-12 Issue:3 Volume:475 Page:4104-4121
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Chon Sunmyon¹,Hosokawa Takashi²,Yoshida Naoki¹³

Affiliation:

1. Department of Physics, School of Science, University of Tokyo, Bunkyo, Tokyo 113-0033, Japan

2. Department of Physics, Kyoto University, Kyoto 606-8502, Japan

3. Kavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo, Chiba 277-8583, Japan

Funder

Japan Society for the Promotion of Science

Ministry of Education

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/475/3/4104/23965850/sty086.pdf

Reference82 articles.

1. Properties of the Binary Black Hole Merger GW150914

2. Photon‐conserving Radiative Transfer around Point Sources in Multidimensional Numerical Cosmology

3. Ubiquitous seeding of supermassive black holes by direct collapse

4. Inspiral-Merger-Ringdown Waveforms for Black-Hole Binaries with Nonprecessing Spins

5. Low-frequency gravitational-wave science with eLISA/NGO

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