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：
暂无
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.
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页码：77 / 80
页数：3
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