XMM-Newton Proposal 03045703

Details XMM-Newton Proposal 03045703 XMM-Newton Proposal 03045703

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..155g&link_type=abstract

XMM-Newton Proposal ID #03045703

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Pg1259+593, Xmm-Newton Proposal 03045703

Scientific paper

We propose to observe three quasars with large CIV emission-line blueshifts to identify and characterize their intrinsic absorption. XMM-Newton spectroscopy will provide a crucial test of the hypothesis that large CIV blueshift quasars are viewed with an orientation angle close to the line-of-sight of a disk wind producing the UV emission lines. Of our three targets, two have already shown evidence for X-ray absorption from exploratory Chandra observations. The third target, PG 1259+593, offers the potential for the first detailed absorption study of this class of quasar.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 03045703 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 XMM-Newton Proposal 03045703, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 03045703 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1474299