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- W2068302015 abstract "The observed rapid radio variations in BLO 0716 +71 can be interpreted in terms of interstellar scintillation, but it requires the source to contain a compact component with angular radius less than ∼ 0.1 - 0.05 mas and the scattering medium to be located nearer than ∼ 0.4kpc. The change from a ‘fast mode’ of variation to a ‘slow mode’ possibly means a change in the state of motion of the compact component. The correlation between the radio and optical variations remains a serious difficulty in this interpretation." @default.
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- W2068302015 title "Interstellar scintillation and fast radio variations in BLO 0716 +71" @default.
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- W2068302015 doi "https://doi.org/10.1016/0275-1062(95)00011-g" @default.
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