Insight in the Emission Mechanisms of the Brightest ULX in the Cartwheel

Details Insight in the Emission Mechanisms of the Brightest ULX in the Cartwheel Insight in the Emission Mechanisms of the Brightest ULX in the Cartwheel

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010head...11.4220w&link_type=abstract

American Astronomical Society, HEAD meeting #11, #42.20; Bulletin of the American Astronomical Society, Vol. 41, p.728

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Scientific paper

The compact X-ray source N10 detected in the Cartwheel ring is one of the brightest ULXs in the sky. I will present results on the variability of this source, and its spectrum. I will discuss the inferred parameters in the context of the current theoretical models. Due to the low statistics, we cannot clinch down the argument on the nature of N10. Nonetheless, I will show that the available information allow us to constrain the parameter space for black hole accretion.

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