41 rotation energy levels / 40 radiative transitions / 210 collisional transitions for para-H2 (17 temperatures in the range 5-300K) / 210 collisional transitions for ortho-H2 (17 temperatures in the
Collisional excitation rate coefficients play an important role in the dynamics of energy transfer in the interstellar medium. In particular, accurate rotational excitation...
Knowledge of rotational energy transfer (RET) involving carbon monoxide (CO) molecules is crucial for the interpretation of astrophysical data. As of now, our nearly perfect understanding of atom-mole