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

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cxo..prop.2076t&link_type=abstract

Chandra Proposal ID #08700001, p.1

Physics

Chandra Proposal Id #08700001

Scientific paper

Recent advances have shown X-ray flux to be simply correlated with reflection-signatures from the disk and with an associated wind in AGN. 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 is currently in a very high state, which we predict will lead to observable features from the disk and its wind. UV data indicate NGC 3516 is very likely to have an observable disk wind due to a favorable orientation. We request 210 ks XMM exposure on NGC 3156 with supporting 200 ks Chandra time to test our prediction of flux-linked disk reflection and wind.

Affiliated with

Also associated with

No associations

Rating

NGC 3516: Disk Diagnostics from a Windy BLSy1 in a High-State does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with NGC 3516: Disk Diagnostics from a Windy BLSy1 in a High-State, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and NGC 3516: Disk Diagnostics from a Windy BLSy1 in a High-State will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-998003