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Session 11 - AGN.
Display session, Monday, January 13
Metropolitan Ballroom,
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
