DNC
Deuterium isocyanide
Species tag 028508
Version2*
Date of EntrySep. 2009
ContributorH. S. P. Müller

New low-J data, to a considerable part with resolved 14N and D hyperfine structure, have been employed with respect to the Nov. 2005 entry. The J" = 0 transition was taken from astronomical observations by
(1) F. F. S. van der Tak, H. S. P. Müller, M. E. Harding, and J. Gauss, 2009, Astron. Astrophys., accepted;
the J" = 0 to 2 transitions were taken from laboratory measurements by
(2) H. A. Bechtel, A. H. Steeves, and R. W. Field, 2006, Astron. Astrophys. 649, L53;
the J" = 3 transition was taken from
(3) T. Okabayashi and M. Tanimoto, 1993, J. Chem. Phys. 99, 3268;
the remaining transitions up to 2 THz were published by
(4) S. Brünken, H. S. P. Müller, S. Thorwirth, F. Lewen, and G. Winnewisser, 2006, J. Mol. Struct. 380–381, 3.
The predictions should be reliable up to at least 2.5 THz.
At low J, the 14N and D hyperfine splitting has been resolved in astronomical observations. Therefore, a separate hyperfine calculation up to J" = 2 is provided along with appropriate partition function values. The dipole moment was assumed to agree with that of HNC, see e027502.cat.

Lines Listed39
Frequency / GHz< 2960
Max. J39
log STR0-5.0
log STR1-4.0
Isotope Corr.-3.946
Egy / cm–10.0
 µa / D3.05
 µb / D 
 µc / D 
 A / MHz 
 B / MHz38152.99
 C / MHz 
 Q(300.0)164.2705
 Q(225.0)123.2682
 Q(150.0)82.2782
 Q(75.00)41.3009
 Q(37.50)20.8181
 Q(18.75)10.5803
 Q(9.375)5.4669
 Q(5.000)3.0903
 Q(2.725)1.8734
detected in ISM/CSMyes


Database maintained by Holger S. P. Müller and Sven Thorwirth, programming by D. Roth and F. Schloeder