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Detecting Direct Collapse Black Holes: making the case for CR7

, , , , , , and . (2015)cite arxiv:1510.01733Comment: 7 pages, 4 figures. Submitted to MNRAS.

Abstract

We propose that one of the sources in the recently detected system CR7 by Sobral et al. (2015) through spectro-photometric measurements at $z = 6.6$ harbors a direct collapse blackhole (DCBH). We argue that the LW radiation field required for direct collapse in source A is provided by sources B and C. By tracing the LW production history and star formation rate over cosmic time for the halo hosting CR7 in a $Łambda$CDM universe, we demonstrate that a DCBH could have formed at $z20$. The spectrum of source A is well fit by nebular emission from primordial gas around a BH with MBH $4.4 10^6 \ M_ødot$ accreting at a 40% of the Eddington rate, which strongly supports our interpretation of the data. Combining these lines of evidence, we argue that CR7 might well be the first DCBH candidate.

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[1510.01733] Detecting Direct Collapse Black Holes: making the case for CR7

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