Searching for AGN signatures in IRAS galaxies

Details Searching for AGN signatures in IRAS galaxies Searching for AGN signatures in IRAS galaxies

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..69..558m&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 69, Issue 1-3, p. 558-559.

Physics

Nuclear Physics

Scientific paper

A number of IRAS galaxies appears rather luminous at X-rays, which could be due to the presence of an active nucleus that otherwise is obscured. X-ray observations offer suitable opportunities for detailed spatial and spectral analyses of these galaxies, which will allow to assess whether they possess active nuclei. We are currently working on ROSAT, ASCA and possibly SAX data of several such galaxies.

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