How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes

M. A. Latif; S. Bovino; T. Grassi; D. R. G. Schleicher; M. Spaans

doi:10.1093/mnras/stu2244

How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes

M. A. Latif, S. Bovino, T. Grassi, D. R. G. Schleicher, M. Spaans

Astrofysik og Planetforskning

60 Citationer (Scopus)

Originalsprog	Engelsk
Tidsskrift	Monthly Notices of the Royal Astronomical Society
Vol/bind	446
Udgave nummer	3
Sider (fra-til)	3163-3177
ISSN	0035-8711
DOI	https://doi.org/10.1093/mnras/stu2244
Status	Udgivet - 21 jan. 2015

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10.1093/mnras/stu2244

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title = "How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes",

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author = "Latif, {M. A.} and S. Bovino and T. Grassi and Schleicher, {D. R. G.} and M. Spaans",

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AU - Latif, M. A.

AU - Bovino, S.

AU - Grassi, T.

AU - Schleicher, D. R. G.

AU - Spaans, M.

PY - 2015/1/21

Y1 - 2015/1/21

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KW - galaxies: formation

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KW - early Universe

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DO - 10.1093/mnras/stu2244

M3 - Journal article

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JF - Royal Astronomical Society. Monthly Notices

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How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes

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