Carbon and oxygen X-ray line emission from the interstellar medium

Details Carbon and oxygen X-ray line emission from the interstellar medium Carbon and oxygen X-ray line emission from the interstellar medium

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...253..131s&link_type=abstract

Astrophysical Journal, Part 1, vol. 253, Feb. 1, 1982, p. 131-135. Research supported by the Centre National d'Etudes Spatiales

Astronomy and Astrophysics

Astronomy

21

Carbon, Interstellar Matter, Oxygen Ions, X Ray Spectra, Spaceborne Astronomy, Supernovae

Scientific paper

A soft X-ray, 0.3-1.0 keV spectrum from a 1 sr region which includes a portion of the North Polar Spur, obtained by three rocketborne lithium-drifted silicon detectors, shows the C V, C VI, O VII and O VIII emission lines. The spectrum is well fitted by a two-component, modified Kato (1976) model, where the coronal emission is in collisional equilibrium, with interstellar medium and North Polar Spur temperatures of 1.1 and 3.8 million K, respectively.

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