Implications of ROSAT observations for the local hot bubble

Details Implications of ROSAT observations for the local hot bubble Implications of ROSAT observations for the local hot bubble

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..103s&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 13, no. 12, p. (12)103-(12)111

Astronomy and Astrophysics

Astronomy

6

Astronomical Models, Background Radiation, H I Regions, Interstellar Matter, Molecular Clouds, Shadows, Sky Surveys (Astronomy), X Ray Astronomy, Galactic Halos, Proportional Counters, Pulsars, Rosat Mission, X Ray Telescopes

Scientific paper

The ROSAT all-sky survey and Guest Observer pointed observations have brought a wealth of high-quality data to the study of the soft X-ray diffuse background. Analysis of the spatial structure of the 1/4 keV flux, including observations of shadows cast by discrete clouds in the interstellar medium, have allowed the separation of the observed flux into foreground and background components supporting a spatially varying local component consistent with previous ideas of the local hot bubble, a highly variable galactic halo component, and an extragalactic background.

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