Abstract
We present subarcsecond MERLIN 0.4-GHz (73 cm) and 1.6-GHz (18 cm) radio measurements of the nuclear region of the Seyfert galaxy NGC 4151. By comparison with higher frequency observations, we deduce that one component (C4) shows a low-frequency turnover which we interpret as evidence for free-free absorption by ionized gas with an emission measure between 3 × 105 and 106 pc cm-6. The free-free absorption appears to be localized to a region ∼50 pc in extent, and we consider models in which the ionized gas may be closely associated with a neutral molecular torus.
| Original language | English |
|---|---|
| Pages (from-to) | 1071-1076 |
| Number of pages | 6 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 300 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 11 Nov 1998 |
| Externally published | Yes |
Keywords
- Galaxies: Seyfert
- Galaxies: individual: NGC 4151
- Galaxies: nuclei
- Radio continuum: galaxies