English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We calculated the polarization degree of hydrogen Balmer broad emission linesfrom a number of active galactic nuclei (AGNs) with determined virial factors.The objects were selected from the sample presented by Decarli et al.(2008). Inour calculations, we used the model of the flattened disc-like structure of thebroad-line emission region (BLR). In this model, the expression for the virialfactor makes it possible to determine the inclination angle for the flattenedBLR, which in turn yields the polarization degree of the broad emission lines.As a result, we obtained the direct relation between the polarization degreeand the virial factor. We also compared the determined values of thepolarization degree with those obtained in polarimetric observations.

Polarization of broad line emission from AGNs with determined virial factors