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- W2000535514 abstract "There is little information concerning the azimuthal distribution of X-rays in dust-scattering halos. This paper describes a Chandra observation of the bright source Cyg X-2 designed specifically for this purpose. After measuring and subtracting ≈10% instrument effects, we find the scattering halo to be rather uniform with possible fluctuations in the surface brightness of only 2%. Observations and data processing are discussed in detail. Some information about the dust distribution is derived." @default.
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- W2000535514 date "2013-04-30" @default.
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- W2000535514 title "AZIMUTHAL STRUCTURE OF THE Cyg X-2 X-RAY DUST HALO" @default.
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- W2000535514 doi "https://doi.org/10.1088/0004-637x/769/1/17" @default.
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