@Article{PereiraMira:2014:AcHiAc,
author = "Pereira, Eduardo dos Santos and Miranda, Oswaldo Duarte",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Accretion history of active black holes from type 1 AGN",
journal = "Astrophysics and Space Science",
year = "2014",
volume = "352",
number = "2",
pages = "801--807",
keywords = "black hole physics, galaxies, quasars.",
abstract = "Almost all galaxies have massive central black holes in their
centers with masses typically ranging from ~105 to ~109 M.
However, the origin and evolution of these objects and their
connection with the hosting galaxies are not completely understood
yet. In this work we analyze the mass accretion rate of
supermassive black holes (SMBH's) and the mean Eddington ratio
(MER) of type 1 AGN using data from the Sloan Sky Survey. For this
purpose we improve the method for constructing the subsample of
SMBH, taking into account the survey flux limit and the bias of
the sample. It was observed that the mean bolometric luminosity of
the active black holes can be represented by a function composed
by a power law in mass and a like-Schechter function in redshift.
Our results also show that both the mean Eddington ratio and the
mass accretion rate are proportional to this function. © 2014
Springer Science+Business Media Dordrecht.",
doi = "10.1007/s10509-014-1934-7",
url = "http://dx.doi.org/10.1007/s10509-014-1934-7",
issn = "0004-640X",
label = "scopus 2014-11 PereiraMira:2014:AcHiAc",
language = "en",
targetfile = "pereiamirana2014_Final.pdf",
urlaccessdate = "27 abr. 2024"
}