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- W1994865779 abstract "We have used 2 Micron All Sky Survey (2MASS) mapping results to investigate the distribution of hot dust continua in 12 planetary nebulae (PNe). The nature of this emission is unclear, but it is possible that where the continuum is extended, as is the case for M 1-12 and NGC 40, then the grains concerned may be very small indeed. The absorption of individual photons by such grains may lead to sharp spikes in temperature, as has previously discussed for several other such outflows. Other sources (such as MaC 1-4, He 2-25, B1 2-1 and K 3-15) appear to be relatively compact, and the high temperatures observed are understandable in terms of more normal heating processes. It is possible that the grains in these cases are experiencing high radiant flux levels." @default.
- W1994865779 created "2016-06-24" @default.
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- W1994865779 date "2006-06-01" @default.
- W1994865779 modified "2023-09-25" @default.
- W1994865779 title "Further 2MASS mapping of hot dust in planetary nebulae" @default.
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- W1994865779 doi "https://doi.org/10.1111/j.1365-2966.2006.10237.x" @default.
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