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On the efficiency of production of the Fe Kalpha emission line in neutral matter

Abstract:

The absolute luminosity of the Fe Kalpha emission line from matter illuminated by X-rays in astrophysical sources is nontrivial to calculate except when the line-emitting medium is optically-thin to absorption and scattering. We characterize the Fe Kalpha line flux using a dimensionless efficiency, defined as the fraction of continuum photons above the Fe K shell absorption edge threshold energy that appear in the line. The optically-thin approximation begins to break down even for column den...

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Publication status:
Published

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
Journal:
Monthly Notices of the Royal Astronomical Society
Volume:
401
Issue:
1
Pages:
411-417
Publication date:
2009-09-04
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Language:
English
Keywords:
Pubs id:
pubs:41466
UUID:
uuid:1e998d83-3c4b-44b7-a8ac-d433c023277e
Local pid:
pubs:41466
Source identifiers:
41466
Deposit date:
2012-12-19

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