Geometrical and chemical dependence of K-shell X-ray features

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

72

Line: Formation, Line: Profiles, Radiative Transfer, Galaxies: Active, X-Rays: Galaxies, X-Rays: Stars

Scientific paper

We review and discuss the chemical and geometrical dependence of iron K features (emission line and absorption edge), and of fluorescent lines from other elements, emitted by neutral, externally X-ray-illuminated matter. Our aim is to provide simple, practical tools which could be useful for observers in order to estimate parameters easily from measured quantities. The dependence of the iron fluorescent line on the iron and oxygen abundances is explored in detail, and simple analytical formulae are given for both the Morrison & McCammon and Anders & Grevesse abundances. In the latter case, the variation of the depth of the iron K edge with the iron abundance is also shown. Fluorescent line intensities from other elements, from oxygen to nickel, are also given as a function of the inclination angle and chemical abundances. The effects of the presence of a hot corona above the cold matter on the iron line and edge are discussed. We also discuss the spectral signature of resonant transitions occurring in the hot corona itself. The present calculations are relevant to AGN and Galactic X-ray binaries, in particular black hole candidates and cataclysmic variables.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Geometrical and chemical dependence of K-shell X-ray features 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 Geometrical and chemical dependence of K-shell X-ray features, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Geometrical and chemical dependence of K-shell X-ray features will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1415200

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.