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H. Feng, P. Kaaret (Department of Physics and Astronomy, The University of Iowa)
We examined X-ray spectral and timing properties of bright ultra-luminous X-ray sources (ULXs) in nearby galaxies with XMM-Newton archival data. For those sources with prominent thermal components, a correlation was found between the X-ray luminosity and the thermal temperature except three special objects whose spectra could also be fitted by a single Comptonization model. Timing noise above the Poisson level was detected from eight sources. We discussed interpretation of these ULXs as accreting intermediate mass black holes.
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Bulletin of the American Astronomical Society, 37 #2
© 2005. The American Astronomical Soceity.