Abstract
Spectropolarimetry was used to study eight high-polarization Seyfert 2 galaxies. In four of them (Mrk 3, Mrk 348, Mrk 463E, and NGC 7674), evidence was found for a hidden broad-line region (BLR), visible only in the polarized flux spectrum. The other four objects, Mrk 78, Mrk 1066, NGC 591, and NGC 7672, may also have hidden BLRs, but at a flux level below the detection threshold. The properties of the hidden BLRs are consistent with their normal Seyfert 1 nuclei. If all Seyfert 2 galaxies are in reality Seyfert 1 galaxies in which the nuclei are hidden from direct view and seen only in scattered light, then one might expect that many Seyfert 2 galaxies have polarizations of their featureless continua greater than 50 percent. Such high polarization are not seen, perhaps indicating a particular geometry, in which nearly edge-on obscuring tori also block light from the scattering region. This model predicts that, in edge-on cases, little or no featureless continua in the spectra of the objects will be detected. Arguments are presented that objects with high luminosity, such as QSOs, have geometrically thin tori and hence are much less likely to have obscured continua and BLRs. 49 refs.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
