Spectral analysis of the jet in the Seyfert 2 Galaxy NGC 6217 with XMM-Newton

Details Spectral analysis of the jet in the Seyfert 2 Galaxy NGC 6217 with XMM-Newton Spectral analysis of the jet in the Seyfert 2 Galaxy NGC 6217 with XMM-Newton

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...37p&link_type=abstract

XMM-Newton Proposal ID #04009202

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Ngc 6217, Ngc 6217, Xmm-Newton Proposal 04009202

Scientific paper

The nuclear starburst, flat spectrum spiral NGC6217 offers the possibility to resolve spectrally with XMM-Newton its one-sided jet-like radio and X-ray filament, extending out to 2.7' (18.8 kpc) in the SW of the galaxy. According to ROSAT observations, the jet's X-ray spectrum seems to be harder than that of NGC6217 and its luminosity in the 0.5-2.0 keV band ~1.7 10E39 erg/s. NGC6217 stands out as the fourth nearest jet galaxy known. Here, we propose a deep XMM-Newton observation of this extraordinary source to resolve the jet from the emission of the galaxy and do a detailed spectral investigation of the jet.

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