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- W2012189931 abstract "The 10.8-micron images of Comet Tempel 2 obtained on the four days from September 21 to 24, 1988, indicate that the dust coma contributed about half of the nuclear pixel brightness. The nuclear condensation brightness exhibited a temporal variability slightly larger than observational uncertainty. The structure of the observed extended dust emission is interpretable as (1) a large grain tail primarily generated by cm-scaled particles, (2) the result of an outburst near 2.5-3.0 AU perihelion, and (3) a sunward emission of dust in a fanlike pattern." @default.
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- W2012189931 date "1990-07-01" @default.
- W2012189931 modified "2023-09-27" @default.
- W2012189931 title "Ground-based thermal IR images of comet tempel 2" @default.
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- W2012189931 doi "https://doi.org/10.1016/0019-1035(90)90210-z" @default.
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