Simulated spectral evolution of black holes

DOI

Massive black hole (MBH) seeds at redshift z>~10 are now thought to be key ingredients to explain the presence of the supermassive (10^9-10^M_{sun}) black holes in place ~6 MBH mass density of {rho}{blackdot}<~2.5x10^2^M{sun}/Mpc^3^ assuming standard Eddington-limited accretion. If accretion occurs in the slim disc mode the limits are much weaker, {rho}{blackdot}<~7.6x10^3^M{sun}_/Mpc^3^ in the most constraining case.

Identifier
DOI http://doi.org/10.26093/cds/vizier.74543771
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/454/3771
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/454/3771
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/454/3771
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/454/3771
Provenance
Creator Pacucci F.; Ferrara A.; Volonteri M.; Dubus G.
Publisher CDS
Publication Year 2016
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics