XMM-Newton view of the relativistic Fe Kα feature in the intermediate Seyfert galaxy 4U 1344-60

Details XMM-Newton view of the relativistic Fe Kα feature in the intermediate Seyfert galaxy 4U 1344-60 XMM-Newton view of the relativistic Fe Kα feature in the intermediate Seyfert galaxy 4U 1344-60

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..924..789j&link_type=abstract

THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. AIP Conference Proceedings, Volume 924, pp. 789-794

Computer Science

Active And Peculiar Galaxies And Related Systems, X-Ray Sources, X-Ray Bursts

Scientific paper

XMM-Newton data analysis of the bright galaxy 4U 1344-60 is presented. The observed X-ray spectrum is complex. The continuum emission can be described as a power law obscured by two neutral absorption components. Interestingly, 4U 1344-60 exhibits a broad and skewed iron line at 6.4 keV most likely originated in a few gravitational radius from the black hole. Optical spectral analysis was also presented. On the basis of its results, we propose to classify 4U 1344-60 as a Seyfert 1.5 galaxy located at z=0.012+/-0.001.

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