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- W4248522903 abstract "It is suggested that molecular observations of interstellar clouds can be used to determine the stage of cloud evolution. However, before observational data can reliably be used to investigate the evolutionary path leading from a tenuous cloud of gas and interstellar dust to a star cluster, mechanisms of molecular formation, excitation, and destruction must be taken into account. The evidence is growing that interstellar dust grains have an important role in molecular formation and destruction." @default.
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- W4248522903 date "1973-01-01" @default.
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- W4248522903 title "Some Implications of the Distribution of Interstellar Molecules" @default.
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- W4248522903 doi "https://doi.org/10.1017/s0074180900054486" @default.
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