Observation of features in the soft X-ray background flux

Details Observation of features in the soft X-ray background flux Observation of features in the soft X-ray background flux

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974apj...193l.133w&link_type=abstract

Astrophysical Journal, vol. 193, Nov. 1, 1974, pt. 2, p. L133-L137.

Computer Science

Sound

121

Background Radiation, Galactic Radiation, Radiant Flux Density, Rocket Sounding, X Ray Astronomy, Astronomical Maps, Early Stars, Hydrogen, Interstellar Radiation

Scientific paper

Two rocket observations of very soft X-ray diffuse intensity show three emission regions of large angular extent. A large portion of the sky as seen with wide angular resolution is mapped. These three regions coincide with broad regions of small column densities of neutral hydrogen. It is suggested that a component of the interstellar medium is very hot and is responsible for the soft X-ray emission and the O VI.

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