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- W52962726 abstract "We have calculated the energy loss rate coefficients for water in interstellar molecular clouds. For para-H 2 O, we considered 10 rotational levels connected by 16 radiative transitions and the calculations were done for the kinetic temperature up to 100 K. For ortho-H 2 O, 31 rotational levels connected by 92 radiative transitions were considered and the calculations were done for the kinetic temperature up to 300 K. For the numver density of molecular hydrogen, n H , up to 10 6 cm −3 , the coefficients were found to be independent of n H2 . The coefficients are expressed in the analytical forms as a function of kinetic temperature in the cloud" @default.
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- W52962726 date "1992-01-01" @default.
- W52962726 modified "2023-09-23" @default.
- W52962726 title "Energy loss rates for water in molecular clouds" @default.
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