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- W4233102020 abstract "Abstract Evidence is presented to suggest that the shocked molecular hydrogen emission in the brightest part of the Orion outflow is produced in a J-shock and not a C-shock; that this is true throughout the entire flow; that it may be true in many outflow sources; and that this exacerbates problems with current explanations of the very wide velocity profiles observed in molecular hydrogen emission." @default.
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- W4233102020 date "1989-01-01" @default.
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- W4233102020 title "The Nature of Shocks in Molecular Clouds" @default.
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- W4233102020 doi "https://doi.org/10.1017/s0252921100023460" @default.
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