O13C34S
Carbonyl sulfide, 13C, 34S isotopomer
Species tag 063502
Version1*
Date of EntryApr. 2005
ContributorH. S. P. Müller

The experimental lines are from
(1) A. G. Maki and D. R. Johnson, 1973, J. Mol. Spectrosc. 47, 226; from
(2) A. Dubrulle, J. Demaison, J. Burie, and D. Boucher, 1980, Z. Naturforsch. 35a, 471; from
(3) A. V. Burenin, E. N. Karyakin, A. F. Krupnov, S. M. Shapin, and A. N. Val'dov, 1981, J. Mol. Spectrosc. 85, 1; and from
(4) J.-U. Grabow and W. Stahl, 1990, Z. Naturforsch. 45a, 1043.
Predictions beyond J = 60 should be viewed with some caution.
The 13C nuclear spin-rotation splitting may be resolved for the J = 1 – 0 transition; the splitting is about 5.0 kHz for this transition with an intensity ratio of 1 : 2 (4). This splitting is unlikely to be resolved for higher J because it is only about 3.4 kHz between the strong hfs components. The 13C spin multiplicity of 2 was not considered in the calculation of the partition function !
The dipole moment was derived from
(5) K. Tanaka, T. Tanaka, and I. Suzuki 1985, J. Chem. Phys. 82, 2835.

Lines Listed99
Frequency / GHz< 1166
Max. J99
log STR0-6.5
log STR1-5.6
Isotope Corr.-3.34
Egy / (cm-1)0.0
 µa / D0.7155
 µb / D 
 µc / D 
 A / MHz 
 B / MHz5911.73
 C / MHz 
 Q(500.0)1763.9438
 Q(300.0)1058.1863
 Q(225.0)793.6351
 Q(150.0)529.1426
 Q(75.00)264.7089
 Q(37.50)132.5142
 Q(18.75)66.4227
 Q(9.375)33.3791
detected in ISM/CSMno


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