H2CND
Iminomethane, methanimine, isotopolog with D at N
Species tag 030515
Version1*
Date of EntryMay 2014
ContributorK. Kobayashi
H. S. P. Müller

Transition frequencies were reported by
(1) Y. Motoki, F. Isobe, H. Ozeki, and K. Kobayashi, 2014, Astron. Astrophys. 566, Art. No. A28.
Also included in the analysis were most data from
(2) R. Pearson, Jr. and F. J. Lovas, 1977, J. Chem. Phys. 66, 4149.
Data with uncertainties of 100 kHz or more were not merged. The predictions should be accurate enough for all radioastronomical observations. Specifically, predictions with uncertainties larger than 0.3 MHz should be viewed with some caution.
14N hyperfine splitting may matter in astronomical observations. Therefore, a separate hyperfine calculation is provided for J' ≤ 20 and Ka' ≤ 5 up to 1 THz. NOTE: The partition function does take into account the spin multiplicity of the 14N nucleus !
The dipole moment components were derived in (1) from those of the main species reported by
(3) M. Allegrini, J. W. C. Johns, and A. R. W. McKellar, 1979, J. Chem. Phys. 70, 2829.

Lines Listed1979
Frequency / GHz< 2000
Max. J37
log STR0-7.5
log STR1-5.0
Isotope Corr.-3.814
Egy / cm–10.0
 µa / D1.23
 µb / D1.54
 µc / D 
 A / MHz157673.92
 B / MHz32069.01
 C / MHz28706.33
 Q(300.0)7195.0598
 Q(225.0)4673.2133
 Q(150.0)2544.9135
 Q(75.00)901.8737
 Q(37.50)320.6043
 Q(18.75)114.6449
 Q(9.375)41.4823
 Q(5.000)16.8893
 Q(2.725)7.7500
detected in ISM/CSMno


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