MCG-02-14-009: probing relativistic FeK line and searching light bending effect

Details MCG-02-14-009: probing relativistic FeK line and searching light bending effect MCG-02-14-009: probing relativistic FeK line and searching light bending effect

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop...56p&link_type=abstract

XMM-Newton Proposal ID #05016701

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Mcg-02-14-009, Xmm-Newton Proposal 05016701

Scientific paper

Our previous analysis of a short 5ks XMM-Newton observation of the Seyfert 1 MCG-02-14-009 (z=0.028) has shown that of the lower luminosity Seyfert (L_2-10keV= 6.2e42 erg/s) it has one of the strongest relativistic iron lines (EW 530-770eV). In addition, the spectrum was found to be reflection dominated which seems to indicate that the primary source is located very close to the black hole, where gravitational light bending is important. We propose here to perform a 80ks XMM-Newton observation of this object to determine the physical properties of the innermost environment around supermassive black holes by: a) better contraining the Fe Kalpha line profile. b) searching for line and continuum variability and gravitational light bending effect.

Affiliated with

Also associated with

No associations

Rating

MCG-02-14-009: probing relativistic FeK line and searching light bending effect 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 MCG-02-14-009: probing relativistic FeK line and searching light bending effect, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MCG-02-14-009: probing relativistic FeK line and searching light bending effect will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1022374