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July 1, 1983The Astrophysical Journal1,782 citations

Interstellar photoelectric absorption cross sections, 0.03-10 keV

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RMRichard J. S. MorrisonDMD. McCammon

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Abstract

An effective absorption cross section per hydrogen atom has been calculated as a function of energy in the 0.03-10 keV range using the most recent atomic cross section and cosmic abundance data. Coefficients of a piecewise polynomial fit to the numerical results are given to allow convenient application in automated calculations.

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Cite This Study

Morrison et al. (1983) studied this question.

synapsesocial.com/papers/69fff71010d6befb25775beehttps://doi.org/10.1086/161102
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