X-ray emission from Centaurus A.
Abstract
The X-ray strength of Cen A (NGC 5128) was monitored for 10 years by Vela 5B, beginning in 1979. The 1973 - 1975 period of exceptional activity and strength was especially well covered, and was characterized by numerous rapid changes in intensity, in agreement with other data, indicating that the nucleus of Cen A is small but massive.
- Publication:
-
MPE Report
- Pub Date:
- 1984
- Bibcode:
- 1984MPERp.184..102T
- Keywords:
-
- Radio Galaxies:X Rays;
- X Rays:Radio Galaxies