XMM-Newton Proposal 03033401

Details XMM-Newton Proposal 03033401 XMM-Newton Proposal 03033401

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..124g&link_type=abstract

XMM-Newton Proposal ID #03033401

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Rx J0136.9-3510, Xmm-Newton Proposal 03033401

Scientific paper

We have detected a highly blueshifted (7.6 keV at the source frame) emission feature in the ASCA spectra of the unusual Narrow-line Seyfert 1 galaxy RX J0136.9-3510. At ASCA resolution it is impossible to tell if the feature is a single line or a combination of lines nor if the feature is due to He-like or H-like Fe. The line profile can tell us where the bulk of the emission origin- ates: A low velocity dispersion would favor a wind/outflow origin, while a hi- gher dispersion may allow for an ionized disk reflection origin. Strong absor- ption and resonant scattering could also produce blueshifted line. To acquire better resolution spectrum to constrain the origin of the line via detailed physical modeling, we propose 50 ks XMM-Newton observations of RXJ0136.9-3510.

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