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- W2051208378 abstract "The rate of mass loss in the from of cold dense gas from a wide Wolf-Rayet binary like WR 140 is estimated. At some distance from the binary, this gas can form a dust shell and reradiate the UV radiation in the IR region. In the case of WR 140 which has a high eccentricity the observed IR outbursts may be caused by the strong increase of the cold dense gas outflow from WR 140 at the periastron" @default.
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- W2051208378 date "1991-09-01" @default.
- W2051208378 modified "2023-10-10" @default.
- W2051208378 title "Stellar wind collision and dust formation in long-period, heavily interacting Wolf-Rayet binaries" @default.
- W2051208378 doi "https://doi.org/10.1093/mnras/252.1.49" @default.
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