2011A&A...527A..22I


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.14CEST19:42:13

2011A&A...527A..22I - Astronomy and Astrophysics, volume 527A, 22-22 (2011/3-1)

Low-luminosity AGNs.

ISTOMIN Ya.N. and SOL H.

Abstract (from CDS):

We propose that low-luminosity AGNs (LLAGNs), or some of them, are sources extracting their energy from the black hole rotation by the Blandford-Znajek mechanism. It is shown that almost all energy of the black hole rotation is converted to relativistic protons in a jet. Owing to the high magnetic-field magnitude near the black hole, required for the Blandford-Znajek mechanism, electrons are not strongly accelerated because of their high synchrotron losses. Conversely, protons gain energies on the order of (104-105)mpc2 when crossing the light cylinder surface. Protons are also accelerated in a disk by 2D turbulent motion of the disk matter. We calculate the luminosity of the synchrotron radiation by fast protons in the disk, the frequencies of this radiation being in the infrared band, and the luminosities corresponding to LLAGNs. We measure the very high energy (VHE) radiation luminosities from the disk and the jet, finding that VHE radiation is produced by collisions of accelerated protons with surrounding matter. We predict a correlation between the infrared luminosity LIR and the VHE luminosity LVHE of the disk, LVHE∝LIR1/2M3/2, where M is the mass of a black hole. Two low-luminosity sources Sgr A* and M87, for which luminosities LIR and LVHE are known, appear to follow this scheme. The discovery of new bright VHE sources from LLAGNs could confirm our hypotheses that they are energy sources powered by the Blandford-Znajek mechanism.

Abstract Copyright:

Journal keyword(s): galaxies: active - acceleration of particles - accretion, accretion disks - gamma rays: galaxies

Simbad objects: 5

goto Full paper

goto View the reference in ADS

Number of rows : 5

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 M 87 BiC 12 30 49.42338230 +12 23 28.0438581 10.16 9.59 8.63   7.49 ~ 6213 3
2 NAME Centaurus A Sy2 13 25 27.61509104 -43 01 08.8056025   8.18 6.84 6.66   ~ 3999 3
3 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 3452 3
4 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11542 0
5 HD 226868 HXB 19 58 21.6758193269 +35 12 05.782512305 9.38 9.72 8.91 8.42   O9.7Iabpvar 3925 0

    Equat.    Gal    SGal    Ecl

To bookmark this query, right click on this link: simbad:objects in 2011A&A...527A..22I and select 'bookmark this link' or equivalent in the popup menu


2020.07.14-19:42:13

© Université de Strasbourg/CNRS

    • Contact