Diffuse X-ray emission from the nuclear region and disk of M33

Details Diffuse X-ray emission from the nuclear region and disk of M33 Diffuse X-ray emission from the nuclear region and disk of M33

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000immm.proc..149p&link_type=abstract

The interstellar medium in M31 and M33. Proceedings 232. WE-Heraeus Seminar, 22-25 May 2000, Bad Honnef, Germany. Edited by El

Computer Science

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Scientific paper

Einstein observations of M33 revealed a low surface brightness diffuse X-ray emission component extending out to 10' from the nucleus indicative of a hot ionized interstellar medium of several million K gas. ROSAT observations confirm and substantiate this diffuse disk component. A first analysis of ROSAT HRI observations in addition seemed to indicate extended emission (radius 20 arcsec) for the bright nuclear source (Schulman & Bregman 1995). Our analysis of all ROSAT HRI observations pointing towards the nuclear area of M33 is compatible with a nuclear point source and points at a highly structured interstellar medium in the area south of the nucleus.

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