Article (Scientific journals)
BLR Size in Realistic FRADO Model: The Role of Shielding Effect
Naddaf Moghaddam, Mohammad Hassan; Czerny, Bożena; Szczerba, Ryszard
2020In Frontiers in Astronomy and Space Sciences, 7
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Keywords :
active galaxies; broad line region; dust opacity; FRADO model; shielding effect; Astronomy and Astrophysics; astro-ph.GA; astro-ph.HE
Abstract :
[en] The effective size of broad line region (BLR), so-called the BLR radius, in galaxies with active galactic nuclei (AGN) scales with the source luminosity. Therefore, by determining this location either observationally through reverberation mapping or theoretically, one can use AGNs as an interesting laboratory to test cosmological models. In this article we focus on the theoretical side of BLR based on the Failed Radiatively Accelerated Dusty Outflow (FRADO) model. By simulating the dynamics of matter in BLR through a realistic model of radiation of accretion disk (AD) including the shielding effect, as well as incorporating the proper values of dust opacities, we investigate how the radial extension and geometrical height of the BLR depends on the Eddington ratio [and blackhole mass], and modeling of shielding effect. We show that assuming a range of Eddington ratios and shielding we are able to explain the time-delays in a sample of reverberation-measured AGNs.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Naddaf Moghaddam, Mohammad Hassan  ;  Center for Theoretical Physics, Polish Academy of Sciences, Warsaw, Poland ; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland
Czerny, Bożena;  Center for Theoretical Physics, Warsaw, Poland
Szczerba, Ryszard;  Nicolaus Copernicus Astronomical Center, Torun, Poland
Language :
English
Title :
BLR Size in Realistic FRADO Model: The Role of Shielding Effect
Publication date :
28 April 2020
Journal title :
Frontiers in Astronomy and Space Sciences
eISSN :
2296-987X
Publisher :
Frontiers Media S.A.
Volume :
7
Peer reviewed :
Peer Reviewed verified by ORBi
Funders :
NCN - Narodowe Centrum Nauki
Funding text :
The project was partially supported by National Science Centre, Poland, grant No. 2017/26/A/ST9/00756 (Maestro 9), and by the Ministry of Science and Higher Education (MNiSW) grant DIR/WK/2018/12.
Commentary :
12 pages, 3 figures, Published in Journal of Frontiers in Astronomy and Space Sciences
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