Galactic Line Emission From 1 TO 10 keV

Joseph Silk and Gary Steigman
Phys. Rev. Lett. 23, 597 – Published 15 September 1969
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Abstract

We calculate the flux of x rays produced by low-energy cosmic-ray nuclei in HI regions. We consider electron capture to excited states by cosmic-ray nuclei of heavy elements, followed by cascades down to the ground state. It is found that the electron-capture processes may yield appreciable line intensities in the range 1-10 keV in the galactic plane.

  • Received 28 April 1969

DOI:https://doi.org/10.1103/PhysRevLett.23.597

©1969 American Physical Society

Authors & Affiliations

Joseph Silk and Gary Steigman

  • Institute of Theoretical Astronomy, Cambridge, England

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Issue

Vol. 23, Iss. 11 — 15 September 1969

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