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- W2140368894 abstract "The longest dust trail among those so detected at optical wavelengths was found along the orbit of 4P/Faye in the 2006 return. It extended as long as 10° in the backward direction. The surface brightness increases monotonically with the distance from the nucleus between |$0rlap{.}^circ5$| and 3°, but decreases slowly beyond 4°. The observed brightnesses of the dust trail and the tail are reasonably explained by our dust ejection model. The model shows that the dust trail is composed of cm-sized particles ejected during previous returns, and the derived power indices of the size distribution function of dust particles ejected from the nucleus (|$-$|3.5) and those remaining in the trail (|$-$|1.9) have a big difference for each other. The averaged mass-loss rate (20 kg s|$^{-1}$|) derived from the model is comparable to those of known IRAS dust trail comets." @default.
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- W2140368894 date "2007-08-25" @default.
- W2140368894 modified "2023-10-17" @default.
- W2140368894 title "Detection of a Long-Extended Dust Trail Associated with Short-Period Comet 4P/Faye in 2006 Return" @default.
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- W2140368894 doi "https://doi.org/10.1093/pasj/59.4.l25" @default.
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