Interstellar ultraviolet absorption lines and galactic X-ray sources

Details Interstellar ultraviolet absorption lines and galactic X-ray sources Interstellar ultraviolet absorption lines and galactic X-ray sources

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...211l..29m&link_type=abstract

Astrophysical Journal, vol. 211, Jan. 1, 1977, pt. 2, p. L29-L33.

Astronomy and Astrophysics

Astrophysics

33

Absorption Spectra, Interstellar Matter, Photoionization, Trace Elements, Ultraviolet Spectra, X Ray Sources, Charge Exchange, Gas Density, Interstellar Gas, Ionized Gases

Scientific paper

X-ray photoionization can create zones of highly ionized trace elements in the interstellar gas around a galactic X-ray source. Ultraviolet absorption lines due to the resulting ionic column densities may be observable and may provide information on the environment and age of the X-ray source. The calculated column densities are sensitive to the rates of charge-exchange reactions.

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