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- W2009205122 abstract "A study of the large-scale isotropy of the X-ray background in the energy range 2–18 keV has revealed significant variations in the intensity distribution over the sky |$(,left|b right|,gt,{20}^{^{circ} })$| A galactic component is apparent which contributes between 2.5 and 7.2 per cent of the background between galactic latitudes 90 and 20°, respectively. We find that the most plausible interpretation of this feature is in terms of inverse Compton scattering of starlight and the microwave background by low-energy cosmic ray electrons. We investigate the residual background variations in terms of both 24- and 12-hr effects. A significant oblate 12-hr variation is found. The pole position of this effect |$(l,approx,{245}^{^{circ} },,b,approx, {53}^{^{circ} })$| is coincident, within the errors, with the pole position of the 24-hr anisotropy reported in the microwave background by Smoot, Gorenstein & Muller. We discuss a possible interpretation of this result." @default.
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- W2009205122 date "1980-02-01" @default.
- W2009205122 modified "2023-09-27" @default.
- W2009205122 title "The isotropy of the X-ray background in the energy range 2-18 keV" @default.
- W2009205122 doi "https://doi.org/10.1093/mnras/190.2.243" @default.
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