XMM-Newton Proposal 02037702

Details XMM-Newton Proposal 02037702 XMM-Newton Proposal 02037702

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..196r&link_type=abstract

XMM-Newton Proposal ID #02037702

Other

He 1029-1401, Pg 1416-129, Xmm-Newton Proposal 02037702

Scientific paper

This proposal aims to measure the iron K line profiles in the brightest radio quiet quasars with XMM-Newton. Early XMM-Newton results suggest that the iron line profiles in luminous AGN differ considerably to those in Seyfert 1s, which could be linked to fundamental parameters such as accretion rate and black hole spin. Our aims are to resolve the profiles in all 3 quasars proposed, and determine how the broad line component and thus the accretion disc evolves with luminosity. We will also measure any narrow line component associated with more distant material, such as the torus. Finally we will determine whether a highly ionised outflow is present, which is now being detected in other luminous AGN, and may constitute a substantial fraction of the overall energy budget.

Affiliated with

Also associated with

No associations

Rating

XMM-Newton Proposal 02037702 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 02037702, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and XMM-Newton Proposal 02037702 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1172675