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Optical Polarization of 52 Radio-loud QSO[CLC]s[/CLC] and BL Lacertae Objects

1998/08/07 by Natarajan Visvanathan, Beverley J. Wills, . · 2 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Cosmic Phenomena #Scientific Research and Discoveries #astro-ph

paper · pdf · doi:10.1086/300610

6 pages. Astronomical Journal, in press

arxiv created 1998/08/07 · openalex publication_date 1998/10/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Polarization measurements are presented for 52 radio-loud QSOs and BL Lac objects. For nine highly polarized ( p > 3%) active galactic nuclei (AGNs), these are the first published polarization measurements. Of these nine, seven are highly polarized QSOs (HPQs), one is a BL Lac object, and another is a likely BL Lac object. Polarization variability is confirmed for some of these new and previously known highly polarized AGNs. While six of the HPQs have flat radio spectra and are almost certainly blazars, PKS 1452-217 is probably a new member of the rare class of radio-loud QSOs that show high polarization by scattering, and it is therefore important for testing orientation unified schemes. In competition for the highest redshift HPQ are the well-observed QSO PKS 0438-43 at z = 2.85, with maximum p ∼ 4.7%, and PKS 0046-315 at z = 2.72, for which we find p ∼ 13%.

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