Fe K features as probes of the nuclear reflection region in Seyfert galaxies

Details Fe K features as probes of the nuclear reflection region in Seyfert galaxies Fe K features as probes of the nuclear reflection region in Seyfert galaxies

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...320l...5k&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 320, Sept. 1, 1987, p. L5-L8.

Astronomy and Astrophysics

Astrophysics

160

Electron Scattering, Galactic Nuclei, K Lines, Seyfert Galaxies, X Ray Spectra, Compton Effect, Photoionization

Scientific paper

The warm electron scattering region posited in 1985 by Antonucci and Miller to exist in NGC 1068 may be a characteristic feature of Seyfert galaxies. Whenever it exists, it presents a unique signature in Fe X-ray features. Predictions of the strength of the Fe K-edge and Kα line in both type 1 and type 2 Seyfert galaxies are presented and interpreted.

Affiliated with

Also associated with

No associations

Rating

Fe K features as probes of the nuclear reflection region in Seyfert galaxies 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 Fe K features as probes of the nuclear reflection region in Seyfert galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fe K features as probes of the nuclear reflection region in Seyfert galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1669777