Nonthermal emission from fall-back clouds in the broad-line region of active galactic nuclei

0561510 - FZÚ 2023 RIV GB eng J - Článek v odborném periodiku
Müller, Ana Laura - Naddaf, M.-H. - Zajaček, M. - Czerny, B. - Araudo, Anabella Teresa - Karas, V.
Nonthermal emission from fall-back clouds in the broad-line region of active galactic nuclei.
Astrophysical Journal. Roč. 931, č. 1 (2022), č. článku 39. ISSN 0004-637X. E-ISSN 1538-4357
Grant CEP: GA ČR(CZ) GA20-19854S
Institucionální podpora: RVO:68378271
Klíčová slova: nonthermal emission * active galactic nuclei
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 4.9, rok: 2022
Způsob publikování: Open access

The spectra of active galactic nuclei exhibit broad-emission lines that presumably originate in the broad-line region (BLR) with gaseous-dusty clouds in a predominantly Keplerian motion around the central black hole. Signatures of both inflow and outflow motion are frequently seen. The dynamical character of BLR is consistent with the scenario that has been branded as the failed radiatively accelerated dusty outflow. In this scheme, frequent highvelocity impacts of BLR clouds falling back onto the underlying accretion disk are predicted. The impact velocities depend mainly on the black hole mass, accretion rate, and metallicity, and they range from a few km s−1 up tothousands of km s−1. Formation of strong shocks due to the collisions can give rise to the production of relativistic particles and associated radiation signatures. In this work, the nonthermal radiation generated in this process is investigated, and the spectral energy distributions for different parameter sets are presented. We find that the nonthermal processes caused by the impacts of clouds can lead to emission in the X-ray and the gamma-ray bands, playing the cloud density and metallicity key roles.
Trvalý link: https://hdl.handle.net/11104/0334102