Matches in SemOpenAlex for { <https://semopenalex.org/work/W1491922217> ?p ?o ?g. }
- W1491922217 abstract "The successes and failures of models of interstellar chemistry are discussed with particular reference to molecular clouds, such as Orion, which are in the immediate neighborhood of HII regions. Some recent laboratory measurements at temperatures below 100 K are reviewed and their astrophysical consequences discussed. From a survey of abundance measurements towards Orion, it is concluded that composition differences between hot HII region clouds and cold dark clouds are not great. The influence upon the chemistry of shocks and mass outflow from young protostars is discussed. It is concluded that although some anomalies do exist, gas phase ion-molecule type schemes can account for most of the qualitative features of the observations." @default.
- W1491922217 created "2016-06-24" @default.
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- W1491922217 date "1982-01-01" @default.
- W1491922217 modified "2023-10-17" @default.
- W1491922217 title "Chemistry Relevant to Molecular Clouds near HII Regions" @default.
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- W1491922217 doi "https://doi.org/10.1007/978-94-009-7778-5_48" @default.
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