Spectroscopy and spectropolarimetry of AGN: from observations to modelling

Active galactic nuclei (AGN) are one of the most luminous objects in the Universe, emitting powerful continuum and line emission across all wavelength bands. They represent an important link in the investigations of the galaxy evolution and cosmology. The resolving of the AGN inner structure is stil...

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Veröffentlicht in:arXiv.org 2018-03
Hauptverfasser: Popovic, L C, Ilic, D, Bon, E, Bon, N, Jovanovic, P, Kovacevic, A, Kovacevic-Dojcinovic, J, Lakicevic, M, Marceta-Mandic, S, Rakic, N, Savic, Dj, Simic, S, Stalevski, M
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creator Popovic, L C
Ilic, D
Bon, E
Bon, N
Jovanovic, P
Kovacevic, A
Kovacevic-Dojcinovic, J
Lakicevic, M
Marceta-Mandic, S
Rakic, N
Savic, Dj
Simic, S
Stalevski, M
description Active galactic nuclei (AGN) are one of the most luminous objects in the Universe, emitting powerful continuum and line emission across all wavelength bands. They represent an important link in the investigations of the galaxy evolution and cosmology. The resolving of the AGN inner structure is still a difficult task with current instruments, therefore the spectroscopy and spectropolarimetry are crucial tools to investigate these objects and their components, such as the properties of the supermassive black hole, the broad line region, and the dusty torus. In this review, we present the results of the project "Astrophysical spectroscopy of extragalactic objects", from the observations, data processing and analysis, to the modelling of different regions in AGN.
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subjects Active galactic nuclei
Astronomical models
Cosmology
Data processing
Galactic evolution
Galaxies
Spectrum analysis
Supermassive black holes
Toruses
Universe
title Spectroscopy and spectropolarimetry of AGN: from observations to modelling
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