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- W1611157427 abstract "Recent observations show that infrared reflection nebulae are common phenomena in star forming regions. Extensive observations were made of two nearby infrared reflection nebulae, Orin Molecular Cloud 2 IRS1 (OMC-2/IRS1) and Cepheus A IRS6a (Cep-A/IRS6a). Mie scattering models of ice coated grains were used to study the constraints on the properties and locations of grains that could produce a feature similar to that observed in OMC-2 and Cep-A. It was concluded that scattering by ice particles alone could not be responsible for the 3.1 micron feature observed in infrared reflection nebulae." @default.
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- W1611157427 date "1986-10-01" @default.
- W1611157427 modified "2023-09-23" @default.
- W1611157427 title "The 3.1 micrometer ice band in infrared reflection nebulae" @default.
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