The X-Ray Luminosity of FR Is and FR IIs

Details The X-Ray Luminosity of FR Is and FR IIs The X-Ray Luminosity of FR Is and FR IIs

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..408..309f&link_type=abstract

The Starburst-AGN Connection. ASP Conference Series, Vol. 408, proceedings of the conference held 27-31 October 2008, at Shangha

Astronomy and Astrophysics

Astronomy

Scientific paper

In this paper, the X-ray data are compiled for the X-ray luminosity calculation for 183 radio galaxies (62 FR Is and 121 FR IIs). We found the averaged X-ray luminosity for FRIs is LogLX1KeV=41.84±3.04erg/s, which is lower than that for FR IIs, which is LogLX1KeV=42.43±1.78erg/s. A K-S test indicates that the two groups have different distribution, implying that the X-ray luminosities of the two groups are different.

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