Determination of magnetic fields in broad line region of active galactic nuclei from polarimetric observations

• Magnetic field values that play an important role in broad line region of active galactic nuclei are estimated.
• Estimates of magnetic fields are based on the observed polarization degrees of broad Hα lines and nearby continuum.
• Values of magnetic fields in broad line region for a number of active galactic nuclei are derived.

Magnetic fields play an important role in confining gas clouds in the broad line region (BLR) of active galactic nuclei (AGN) and in maintaining the stability of these clouds. Without magnetic fields the clouds would not be stable, and soon after their formation they would expand and disperse. We show that the strength of the magnetic field can be derived from the polarimetric observations. Estimates of magnetic fields for a number of AGNs are based on the observed polarization degrees of broad Hα lines and nearby continuum. The difference between their values allows us to estimate the magnetic field strength in the BLR using the method developed by Silant’ev et al. (2013). Values of magnetic fields in BLR for a number of AGNs have been derived.