Maximally rotating supermassive stars at the onset of collapse: the perturbative effects of gas pressure, magnetic fields, dark matter, and dark energy-Reference-Cited by-同舟云学术

Maximally rotating supermassive stars at the onset of collapse: the perturbative effects of gas pressure, magnetic fields, dark matter, and dark energy

Published:2018-04-04 Issue:3 Volume:477 Page:3694-3710
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Butler Satya P¹,Lima Alicia R¹,Baumgarte Thomas W¹,Shapiro Stuart L²³

Affiliation:

1. Department of Physics and Astronomy, Bowdoin College, Brunswick, ME 04011, USA

2. Department of Physics, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA

3. Department of Astronomy and NCSA, University of Illinois at Urbana-Champaign, Urbana, IL 61801, USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/477/3/3694/24813073/sty834.pdf

Reference94 articles.

1. Ubiquitous seeding of supermassive black holes by direct collapse

2. Detecting direct collapse black holes: making the case for CR7

3. Metallicity evolution of direct collapse black hole hosts: CR7 as a case study

4. ACCRETION ONTO THE FIRST STELLAR-MASS BLACK HOLES

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