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- W2043455405 abstract "Near-infrared images of the bipolar nebula OH 231.8+4.2 obtained over a 3 yr period suggest that its surface brightness distribution varies with time. A model in which the variations are explained by the differences in travel times for photons scattered off dust grains at various positions along the polar axis of the nebula is presented. This formulation allows us to determine the brightness fluctuations and heliocentric distance of the embedded source and the inclination of the nebula" @default.
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- W2043455405 date "1992-10-01" @default.
- W2043455405 modified "2023-10-18" @default.
- W2043455405 title "Variation in the near-infrared surface brightness distribution of the bipolar nebula OH 231.8 + 4.2" @default.
- W2043455405 doi "https://doi.org/10.1086/171880" @default.
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