Predicted Fe I-III fluxes for AGNs with BLRs

Details Predicted Fe I-III fluxes for AGNs with BLRs Predicted Fe I-III fluxes for AGNs with BLRs

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..222..363s&link_type=abstract

The Interplay among Black Holes, Stars and ISM in Galactic Nuclei, Proceedings of IAU Symposium, No. 222. Edited by T. Storchi-B

Physics

Scientific paper

We present theoretical Fe I-III emission-line strengths for physical conditions typical of Active Galactic Nuclei with Broad-Line Regions. We can satisfactorily reproduce the empirical UV Fe II-III emission-line template of Vestergaard & Wilkes (2001) for the prototypical narrow-line Seyfert 1 galaxy I Zw 1, although a number of detailed discrepancies remain.

Affiliated with

Also associated with

No associations

Rating

Predicted Fe I-III fluxes for AGNs with BLRs 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 Predicted Fe I-III fluxes for AGNs with BLRs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Predicted Fe I-III fluxes for AGNs with BLRs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1113046