N15ND+
Diazenylium, X 1Σ+, deuterated isotopolog with 15N on N2
Species tag 031510
Version1*
Date of EntryMar. 2009
ContributorH. S. P. Müller

The data have been published by
(1) L. Dore, L. Bizzocchi, C. Degle Esposti, and F. Tinti, 2009, Astron. Astrophys. 496, 275.
In order to extrapolate more reliably to higher values of J, a value for the sextic distortion parameter H was derived from DCN, see e028509.cat for references. The predictions are assumed to be reliable to at least 2 THz.
The hyperfine splitting due to the 14N nucleus was derived from N2D+, see e030509.cat. The splitting is probably accurate to better than 5 kHz. A separate hyperfine calculation is provided for J" ≤ 4. Note: The partition function takes into account the14N splitting !
The dipole moment was assumed to be the same as that of the main isotopomer, see e029506.cat.

Lines Listed40
Frequency / GHz< 3026
Max. J40
log STR0-4.0
log STR1-4.0
Isotope Corr.-6.38
Egy / (cm–1)0.0
 µa / D3.40
 µb / D 
 µc / D 
 A 
 B38009.27
 C 
 Q(300.0)494.6327
 Q(225.0)371.1776
 Q(150.0)247.7546
 Q(75.00)124.3651
 Q(37.50)62.6860
 Q(18.75)31.8569
 Q(9.375)16.4587
detected in ISM/CSMno


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