Interstellar deuteroammoniaTracing physical conditions in dense, cold interstellar medium

被引:0
|
作者
D. C. Lis
M. Gerin
E. Roueff
T. G. Phillips
D. R. Poelman
机构
[1] California Institute of Technology,LERMA, UMR 8112 du CNRS
[2] Observatoire de Paris and Ecole Normale Superiéure,LUTH and UMR 8102 du CNRS
[3] Observatoire de Paris,undefined
[4] Section de Meudon,undefined
[5] Kapteyn Astronomical Institute,undefined
来源
Astrophysics and Space Science | 2008年 / 313卷
关键词
ISM: abundances; ISM: molecules; Stars: formation;
D O I
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中图分类号
学科分类号
摘要
Close to 30 deuterated molecules have now been detected in the ISM, including doubly-deuterated species D2H+, ND2H, D2CO, CHD2OH, D2S, and D2CS, as well as triply-deuterated ammonia and methanol. We review the current understanding of depletion and deuteration processes in cold, dense interstellar medium (ISM) and discuss the utility of deuteroammonia as a tracer of the physical conditions and kinematics of cold, dense gas.
引用
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页码:77 / 80
页数:3
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