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- W3184042654 abstract "The all-sky soft X-ray data of McCammon et al. and the new N sub H survey (Stark et al. was used to place limits on the amount of the soft X-ray diffuse background that can originate beyond the neutral gas of the galactic disk. The X-ray data for two regions of the sky near the galactic poles are shown to be uncorrelated with 21 cm column densities. Most of the observed x-ray flux must therefore originate on the near side of the most distant neutral gas. The results from these regions are consistent with X-ray emission from a locally isotropic, unabsorbed source, but require large variations in the emission of the local region over large angular scales." @default.
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- W3184042654 date "1984-05-01" @default.
- W3184042654 modified "2023-09-24" @default.
- W3184042654 title "Limits on soft X-ray flux from distant emission regions" @default.
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