Rotational excitation of mono- and doubly-deuterated water by hydrogen molecules

被引:47
|
作者
Faure, A. [1 ]
Wiesenfeld, L. [1 ]
Scribano, Y. [2 ]
Ceccarelli, C. [1 ]
机构
[1] UJF Grenoble 1, CNRS INSU, IPAG, UMR 5274, F-38041 Grenoble, France
[2] Univ Bourgogne, CNRS, Lab Interdisciplinaire Carnot Bourgogne, UMR 5209, F-21078 Dijon, France
关键词
molecular data; molecular processes; stars: formation; ISM: molecules; INTERSTELLAR HEAVY-WATER; HERSCHEL OBSERVATIONS; SPECTRAL SURVEYS; HDO; TEMPERATURE; ENERGY; H2O; H-2;
D O I
10.1111/j.1365-2966.2011.20081.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Rate 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. A number of potential HDO maser lines are finally identified, in particular the 80.6 GHz (1(1,0)-1(1,1)) transition.
引用
收藏
页码:699 / 704
页数:6
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