The contribution of AGN to the X-ray background: the effect of iron features
- 1 February 1999
- journal article
- Published by Elsevier in New Astronomy
- Vol. 4 (1) , 45-57
- https://doi.org/10.1016/s1384-1076(99)00004-4
Abstract
No abstract availableKeywords
All Related Versions
This publication has 53 references indexed in Scilit:
- Are the Nuclei of Seyfert 2 Galaxies Viewed Face-On?The Astrophysical Journal, 1998
- On the nature of the X-ray absorption in the Seyfert 2 galaxy NGC 4507Monthly Notices of the Royal Astronomical Society, 1998
- ASCAObservations of Type 2 Seyfert Galaxies. II. The Importance of X‐Ray Scattering and ReflectionThe Astrophysical Journal, 1997
- The X-Ray Spectral Variability of Markarian 766The Astrophysical Journal, 1996
- X-Ray Reprocessing by a Molecular Torus in the Seyfert 1.9 Galaxy NGC 2992The Astrophysical Journal, 1996
- The Iron Kα Line Profile in NGC 4151The Astrophysical Journal, 1995
- An ASCA X-Ray Spectrum of a Prototype Bare Seyfert 1 Nucleus in MCG -2-58-22The Astrophysical Journal, 1995
- Iron line emission and two-component spectral behavior in the ASCA observation of the Seyfert 1 galaxy NGC 7469The Astrophysical Journal, 1994
- The X-ray Baldwin effectThe Astrophysical Journal, 1993
- The cosmic x-ray backgroundPhysics Reports, 1987