2010ApJ...711.1174T

We present the detection of extremely broad, double-peaked, highly polarized Hα emission lines in the nuclei of the well-known Seyfert 2 galaxies NGC 2110 and NGC 5252. These hidden broad Hα emission lines, visible only in scattered light, are shown to display significant variability in strength and profile on timescales of ≲1 yr. That the broad emission line exhibits variability in polarized flux also suggests that the scattering region must be very compact, possibly confined in a small number of electron clouds ≲1 lt-yr in size. Our observational constraints place these clouds within ∼10 pc of the nucleus with temperatures T_e≲ 10⁶ K and densities n_e∼ 10⁷/cm3, consistent with a region just outside the obscuring torus between the broad-line region and narrow-line region. These scattering clouds could arise from the clumpy torus itself. These findings and other properties indicate that NGC 2110 and NGC 5252 are the hidden counterparts to the broad-line double-peaked emission-line active galactic nuclei, whose examples include Arp 102B and 3C 332.