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- W2074175035 abstract "The possible contribution of X-ray emission from massive compact objects in the Galactic halo (MACHOs) to the diffuse X-ray background is explored. We show that such emission cannot be responsible for the shadowing seen in soft X-ray observations by ROSAT but that these objects may indeed contribute significantly (at levels greater than 10%) to the diffuse background at higher (greater than or approximately 0.5 keV) energies. Thus, X-ray observations may well be able to significantly constrain the spatial distribution of MACHOs." @default.
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- W2074175035 date "1994-08-01" @default.
- W2074175035 modified "2023-10-16" @default.
- W2074175035 title "MACHOs and the diffuse X-ray background" @default.
- W2074175035 doi "https://doi.org/10.1086/187479" @default.
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