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- W1639144007 abstract "Some possible strong astronomical emission lines in the infrared region are discussed. The line at 12.8 microns, which results from a transition between the fine structure components of the ground state of the ion Ne + , is thought to be emitted from galactic H II regions and also possibly from extended stellar envelopes. The line at 28 microns is emitted in the J = 2 to J = 0 rotational transition in the (para) hydrogen molecule, and could be emitted from interstellar H I regions and from collapsing protostars. Estimates of the expected intensities of these astronomical emission lines are given." @default.
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- W1639144007 date "1965-01-01" @default.
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- W1639144007 title "Infrared emission lines from celestial sources" @default.
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- W1639144007 doi "https://doi.org/10.1017/s0074180900179768" @default.
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