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• W2114067747 abstract "Context. Oxygen molecules (O2) are of particular interest because of their crucial role in astrochemisty. Modelling of O2 molecular emission spectra from interstellar clouds requires the calculation of rate coefficients for excitation by collisions with the most abundant species." @default.
• W2114067747 created "2016-06-24" @default.
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• W2114067747 date "2014-07-01" @default.
• W2114067747 modified "2023-09-30" @default.
• W2114067747 title "Collisional excitation of O₂by H₂: the validity of LTE models in interpreting O₂observations" @default.
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• W2114067747 doi "https://doi.org/10.1051/0004-6361/201423957" @default.
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