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- W3100270939 endingPage "A2" @default.
- W3100270939 startingPage "A2" @default.
- W3100270939 abstract "Context. Recent submillimeter and far-infrared wavelength observations of absorption in the rotational ground-state lines of various simple molecules against distant Galactic continuum sources have opened the possibility of studying the chemistry of diffuse molecular clouds throughout the Milky Way. In order to calculate abundances, the column densities of molecular and atomic hydrogen, H i, must be known." @default.
- W3100270939 created "2020-11-23" @default.
- W3100270939 creator A5008102443 @default.
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- W3100270939 creator A5090822634 @default.
- W3100270939 date "2017-03-17" @default.
- W3100270939 modified "2023-10-17" @default.
- W3100270939 title "Hydrogen in diffuse molecular clouds in the Milky Way" @default.
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