Radio Polarization of BL Lacertae Objects

Details Radio Polarization of BL Lacertae Objects Radio Polarization of BL Lacertae Objects

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..193f&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Astronomy and Astrophysics

Astronomy

Scientific paper

In this paper, using the database of the university of Michigan Radio Astronomy Observatory (UMRAO) at three (4.8 GHz, 8 GHZ, and 14.5 GHz) radio frequencies, we studied the polarization properties for 47 BL Lacertae objects, and found that (1) the polarizations at higher radio frequency is higher than those at lower frequency, and (2) relativistic beaming could explain the polarization characteristic of BL Lacs.

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