Interstellar deuteroammonia. Tracing physical conditions in dense, cold interstellar medium

Details Interstellar deuteroammonia. Tracing physical conditions in dense, cold interstellar medium Interstellar deuteroammonia. Tracing physical conditions in dense, cold interstellar medium

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ap%26ss.313...77l&link_type=abstract

Astrophysics and Space Science, Volume 313, Issue 1-3, pp. 77-80

Astronomy and Astrophysics

Astrophysics

5

Ism: Abundances, Ism: Molecules, Stars: Formation

Scientific paper

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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