NGC 3516: Disk Diagnostics from a Windy BLSy1 in a High-State

Details NGC 3516: Disk Diagnostics from a Windy BLSy1 in a High-State NGC 3516: Disk Diagnostics from a Windy BLSy1 in a High-State

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...49t&link_type=abstract

XMM-Newton Proposal ID #04012103

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Ngc 3516, Ngc 3516, Ngc 3516, Xmm-Newton Proposal 04012103

Scientific paper

Recent advances have shown X-ray flux to be simply correlated with reflection-signatures from the disk and an associated wind. It appears two things are essential to observe the disk/wind: 1) catch the Seyfert in a high-state where disk/wind features show up strongly and 2) separate out reprocessing from distant gas to allow isolation of disk/wind features. NGC 3516 provides the ideal source for further study in this regard. The source is currently in a very high state, which we predict will lead to observable features from the disk and its wind. We request 210 ks XMM exposure on NGC 3156 with supporting Chandra time to test our prediction of flux-linked disk reflection and wind.

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