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• W181744677 abstract "Some techniques for observing shock waves in interstellar clouds are discussed. It is concluded that recent measurements of molecular hydrogen emission provide the best currently available technique for studying shocks. The results of measurements toward the Orion nebula are discussed, and a discussion and summary of the currently known H 2 sources is given." @default.
• W181744677 created "2016-06-24" @default.
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• W181744677 date "1980-01-01" @default.
• W181744677 modified "2023-10-18" @default.
• W181744677 title "Observations of Shock Waves in Interstellar Clouds" @default.
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• W181744677 doi "https://doi.org/10.1017/s0074180900073046" @default.
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