Abstract
The analysis of an INTEGRAL AO2 observation of the error contours of the EGRET source 3EG J1621 + 8203 is presented. The only source found inside the error contours for energies between 20 and 30 keV at 5σ detection significance is the FR I radio galaxy NGC 6251. This supports the identification of NGC 6251 with 3EG J1621 + 8203. The observed flux is higher and softer than observed in the past, but consistent with a variable blazar-like spectral energy distribution.
| Original language | English |
|---|---|
| Pages (from-to) | 515-518 |
| Number of pages | 4 |
| Journal | Astronomy and Astrophysics |
| Volume | 433 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1 Apr 2005 |
Keywords
- Galaxies: active
- Galaxies: individual: NGC 6251
- X-rays: galaxies