A Comparison of X-ray and Radio Observations of NGC 7331
Abstract
We have made deep observations of NGC 7331 using ROSAT and the VLA, at 6 cm and 20 cm. Locations of x-ray and radio sources in the field are compared to previously identified radio and optical sources. X-ray luminosities for identified sources are given and x-ray fluxes are given for unidentified sources. The nucleus of NGC 7331 has been analyzed to discern any new evidence supporting the presence of a massive black hole (MBH). Comparisons are made with other similar sources. Work supported by NASA Grant #NAG5-3214
- Publication:
-
American Astronomical Society Meeting Abstracts
- Pub Date:
- December 1996
- Bibcode:
- 1996AAS...189.1102S