International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 collisions below 300 K are presented. Calculations have been performed at the close-coupling and coupled-states levels with the deuterated variants of the H2O-H-2 interaction potential of Valiron et al. The HDO-H-2 and D2O-H-2 rate coefficients are compared to the corresponding rate coefficients for HDO-He and H2O-H-2, respectively. Significant differences are observed. In particular the new HDO rate coefficients are found to be significantly larger (by up to three orders of magnitude) than the corresponding HDO-He rate coefficients. The impact of the new HDO rate coefficients is examined with the help of non-LTE radiative transfer calculations....
International audienceWater is a key molecule for interstellar chemistry. Observations with Herschel...
Context.The interpretation of water line emission from existing observations and future HIFI/Hersc...
International audienceWater is a key molecule for interstellar chemistry. Observations with Herschel...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceCross sections and rate coefficients for low lying rotational transitions in D...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceAims.Using a newly determined 5D potential energy surface for H2-H2O we provid...
International audienceAims.Using a newly determined 5D potential energy surface for H2-H2O we provid...
International audienceContext: The interpretation of water line emission from existing observations ...
International audienceWater is a key molecule for interstellar chemistry. Observations with Herschel...
Context.The interpretation of water line emission from existing observations and future HIFI/Hersc...
International audienceWater is a key molecule for interstellar chemistry. Observations with Herschel...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceRate coefficients for rotational transitions in HDO and D2O induced by H-2 col...
International audienceCross sections and rate coefficients for low lying rotational transitions in D...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceWe present cross sections and rate coefficients for rotational transitions in ...
International audienceAims.Using a newly determined 5D potential energy surface for H2-H2O we provid...
International audienceAims.Using a newly determined 5D potential energy surface for H2-H2O we provid...
International audienceContext: The interpretation of water line emission from existing observations ...
International audienceWater is a key molecule for interstellar chemistry. Observations with Herschel...
Context.The interpretation of water line emission from existing observations and future HIFI/Hersc...
International audienceWater is a key molecule for interstellar chemistry. Observations with Herschel...