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• W1591129847 abstract "Observations, which have been published since 1979, of molecular species in diffuse clouds will be discussed. Particular attention will be given to the ultraviolet measurements of CO with the Copernicus and IUE satellites and to ground-based optical measurements of CH, CH + , CN, and C 2 . These data encompass large enough samples to test the chemical schemes expected to occur in diffuse clouds. Upper limits for other species (e.g., H 2 O, H 2 O + , and C 3 ) place restrictions on the pathways for molecular production. Moreover, analysis of the rotational distribution of the C 2 molecule results in the determination of the physical conditions of the cloud. These parameters, including density, temperature, and the intensity of the radiation field, are necessary for modeling the chemistry." @default.
• W1591129847 created "2016-06-24" @default.
• W1591129847 creator A5062102157 @default.
• W1591129847 date "1987-01-01" @default.
• W1591129847 modified "2023-10-02" @default.
• W1591129847 title "Optical Observations Related to the Molecular Chemistry in Diffuse Interstellar Clouds" @default.
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• W1591129847 doi "https://doi.org/10.1007/978-94-009-4774-0_23" @default.
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