Abstract
The authors present millimetre, submillimetre, far- and near-infrared observations of the unusual galaxy NGC 1275. After subtracting the near-infrared stellar contamination of the surrounding galaxy they investigate the non-stellar emission at these wavelengths. They conclude that the millimetre-wave and near-infrared emission is synchrotron radiation from a very compact component. The variability properties and radio morphology are similar to 3C 273 and the very active Blazars. It is shown that the emission at wavelengths from 10 - 400 \ensuremath\mu
| Original language | English (Ireland) |
|---|---|
| Number of pages | 9 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 217 |
| Publication status | Published - 1 Jan 1985 |
Authors (Note for portal: view the doc link for the full list of authors)
- Authors
- Walter Kieran Gear and E. I. Robson and G. Gee and I. G. Nolt