Interstellar photoelectric absorption cross sections, 0.03-10 keV

Details Interstellar photoelectric absorption cross sections, 0.03-10 keV Interstellar photoelectric absorption cross sections, 0.03-10 keV

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...270..119m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 270, July 1, 1983, p. 119-122.

Astronomy and Astrophysics

Astronomy

1808

Absorption Cross Sections, Cosmic Dust, Interstellar Chemistry, Interstellar Matter, X Ray Astronomy, Abundance, Electrophotometry, Ionization, Molecules

Scientific paper

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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