Abstract
We present infrared spectroscopy of He I 1.083 μm and Paβ for a sample of nine Seyfert 2 galaxies. These galaxies were selected for strong emission at ∼3 μm and spectral energy distributions similar to type 1 Seyferts. We find broad emission lines components (FWHM ∼1500 km s-1) in six galaxies of our sample and evidence for strong dust obscuration. Spectropolarimetry of Mrk 334 reveals that scattering screens are not a universal component of the broad-line region in Seyfert galaxies. The overall results show that the portion of Seyfert 1 galaxies is underestimated significantly in optically based studies and support current unified models for active galactic nuclei.
Original language | English (US) |
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Pages (from-to) | 608-613 |
Number of pages | 6 |
Journal | Astrophysical Journal |
Volume | 423 |
Issue number | 2 |
DOIs | |
State | Published - Mar 10 1994 |
Keywords
- Galaxies: Seyfert
- Galaxies: active
- Infrared: galaxies
- Polarization
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science