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2015MNRAS.448.2879A - Mon. Not. R. Astron. Soc., 448, 2879-2889 (2015/April-2)
Spectropolarimetric monitoring of active galaxy 3C 390.3 with 6-m telescope SAO RAS in the period 2009-2014.
AFANASIEV V.L., SHAPOVALOVA A.I., POPOVIC L.C. and BORISOV N.V.
Abstract (from CDS):
We find a small lag (10-40 d) between the unpolarized and polarized continuum that is significantly smaller than the estimated lags for the unpolarized broad emission lines (lag(Hα) ∼ 138-186 and lag(Hβ) ∼ 60-79 d). This shows that the region of the variable polarized continuum is significantly smaller than the broad line region, indicating that a part of the polarized continuum is coming from the jet. The lag of the polarized light in the Hα line (89-156 d) indicates an additional component to the disc one that has an outflowing velocity of ∼ - 1200 km/s. This region seems to depolarize the polarized broad Hα line emitted from the disc and scattered in the inner part of the torus.
Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)
Journal keyword(s): line: profiles - galaxies: active - quasars: individual: 3C 390.3
VizieR on-line data: <Available at CDS (J/MNRAS/448/2879): table2.dat>
Simbad objects: 4
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