Abstract
We report the detection of strong, broad Hα emission seen in polarized flux from the early-type radio galaxy IC 5063. This suggests that the galaxy has a broad-line region which is obscured from our direct view, with the broad-line radiation being scattered into our line of sight by scatterers outside the obscuring regions. A model has been developed to estimate the dilution by starlight of the intrinsic polarization, and to correct for interstellar polarization. The FWHM of the broad Hα is 3400 km s^-1^, well within the range covered by typical Seyfert 1 galaxies.
| Original language | English |
|---|---|
| Pages (from-to) | 895-902 |
| Journal | Monthly Notices of the Royal Astronomical Society (MNRAS) |
| Volume | 263 |
| Issue number | 4 |
| Publication status | Published - 1993 |
Fingerprint
Dive into the research topics of 'Evidence for an Obscured Broadline Region in the Early Type Radio Galaxy IC5063'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver