Deconstructing the Soft X-ray Background

Details Deconstructing the Soft X-ray Background Deconstructing the Soft X-ray Background

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000head....5.3226k&link_type=abstract

American Astronomical Society, HEAD Meeting #5, #32.26; Bulletin of the American Astronomical Society, Vol. 32, p.1240

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Scientific paper

Using the 6-band ROSAT All-Sky Survey, the Dwingeloo HI Survey, and the Schelgel et al. (1998) maps of IRAS emission, we have isolated and fit the spectral energy distribution of the galactic halo. We show that the 0.25-2.0 keV band SED of the galactic halo must be composed of at least two thermal components; a patchy component with log T=6.056, and a smoother component with log T=6.426. The hotter component is similar to that seen in external spiral galaxies.

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