The rotational excitation of the water isotopologues by molecular hydrogen

被引:5
|
作者
Faure, A. [1 ]
Zoltowski, M. [2 ,3 ]
Wiesenfeld, L. [4 ]
Lique, F. [3 ]
Bergeat, A. [5 ]
机构
[1] Univ Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
[2] Univ Le Havre Normandie, CNRS, LOMC, F-76600 Le Havre, France
[3] Univ Rennes, CNRS, IPR Inst Phys Rennes, F-35000 Rennes, France
[4] Univ Paris Saclay, CNRS, Lab Aime Cotton, F-91405 Orsay, France
[5] Univ Bordeaux, CNRS, ISM, F-33400 Talence, France
关键词
astrochemistry; line: formation; masers; molecular data; molecular processes; scattering; DISKS; INTERSTELLAR; COLLISION; DATABASE;
D O I
10.1093/mnras/stad3037
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present cross-sections and rate coefficients for rotational transitions in the water isotopologues D2O, (H2O)-O-18, and HDO induced by collisions with para-H-2(j(2) = 0) and ortho-H-2(j(2) = 1). Quantum scattering calculations are performed at the full close-coupling level with the isotopic variants of an accurate full-dimensional H2O-H-2 interaction potential. The D2O, (H2O)-O-18, and HDO cross-sections are compared to the corresponding cross-sections for H2O. Large isotopic effects are observed in the case of D2O and HDO, in particular for collisions with p-H-2(j(2) = 0), while the O-18 isotopic substitution is found to be negligible. Rate coefficients are provided for rotational transitions among all para-D2O, ortho-D2O, and HDO levels with internal energy below 300 cm(-1) and for kinetic temperatures in the range 5-300 K. Non-LTE radiative transfer calculations show that the HDO 225.9 GHz and (H2O)-O-18 203.4 GHz transitions recently detected with ALMA in the young proto-planetary disc V883 Ori should be inverted (weak masers) in a large fraction of the disc.
引用
收藏
页码:3087 / 3093
页数:7
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