Formation of massive seed black holes via collisions and accretion-Reference-Cited by-同舟云学术

Formation of massive seed black holes via collisions and accretion

Published:2018-01-29 Issue:1 Volume:476 Page:366-380
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Boekholt T C N¹²^ORCID,Schleicher D R G¹,Fellhauer M¹,Klessen R S³⁴,Reinoso B¹,Stutz A M¹,Haemmerlé L⁵

Affiliation:

1. Departamento de Astronomía, Facultad Ciencias Físicas y Matemáticas, Universidad de Concepción, Av. Esteban Iturra s/n Barrio Universitario, Casilla 160, Concepción, Chile

2. Departamento de Física, Universidade de Aveiro, CIDMA, Campus de Santiago, P-3810-193 Aveiro, Portugal

3. Universität Heidelberg, Zentrum für Astronomie, Institut für Theoretische Astrophysik, Albert-Ueberle-Str. 2, D-69120 Heidelberg, Germany

4. Universität Heidelberg, Interdisziplinäres Zentrum für Wissenschaftliches Rechnen, Im Neuenheimer Feld 205, D-69120 Heidelberg, Germany

5. Observatoire de Genève, Université de Genève, chemin des Maillettes 51, CH-1290 Sauverny, Switzerland

Funder

Fundação para a Ciência e a Tecnologia

ERC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/476/1/366/24238722/sty208.pdf

Reference75 articles.

1. Revised rate coefficients for H2 and H− destruction by realistic stellar spectra

2. Effects of binary stellar populations on direct collapse black hole formation

3. An analytic resolution to the competition between Lyman–Werner radiation and metal winds in direct collapse black hole hosts

4. An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5

5. The role of stellar collisions for the formation of massive stars

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