Abstract :
[en] We discuss the polarization of broad emission lines in the type 1 active galactic nuclei (AGN). The polarization depends on the geometry of the broad line region (BLR), and also on the polarization mechanism, or distribution of the scattering material. Therefore, the polarization measurements can indicate the geometry of the BLR and the mechanism of polarization (equatorial or polar scattering). In addition, the polarization angle (PA) shape across the line profile can be used to measure the supermassive black hole (SMBH) mass, and constrain the BLR characteristics. We give an overview of ours and other recent investigations of the polarization in broad lines from both aspects: theoretical and observational.
Funding text :
RFBR, 20‐02‐00048; Ministry of Science and Higher Education of the Russian Federation, 05.619.21.0016; Ministry of Education, Science and Technological Development of R. Serbia, 451‐03‐9/2021‐14/200104; 451‐03‐68/2020‐14/200002 Funding informationThis review paper is devoted to the Victor L. Afanasiev who led the observational part of the polarization observations, but also always gave original ideas about the observational effects and their theoretical explanation. This work was supported by Ministry of Education, Science and Technological Development of R. Serbia contracts no. 451‐03‐68/2020‐14/200002 and no. 451‐03‐9/2021‐14/200104. Observations with the SAO RAS telescopes are supported by the Ministry of Science and Higher Education of the Russian Federation (including agreement No 05.619.21.0016, project ID RFMEFI61919X0016). ES was supported by RFBR grant, project number 20‐02‐00048. We would like to thank Professor Hagai Netzer for very useful comments.
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