A Comparison of X-ray and Radio Observations of NGC 7331

Details A Comparison of X-ray and Radio Observations of NGC 7331 A Comparison of X-ray and Radio Observations of NGC 7331

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.1102s&link_type=abstract

American Astronomical Society, 189th AAS Meeting, #11.02; Bulletin of the American Astronomical Society, Vol. 28, p.1287

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Scientific paper

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

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