17OCS
Carbonyl sulfide, 17O isotopomer
Species tag 061504
Version1*
Date of EntryApr. 2005
ContributorH. S. P. Müller

The experimental lines without 17O hyperfine splitting are from
(1) A. Dubrulle, J. Demaison, J. Burie, and D. Boucher, 1980, Z. Naturforsch. 35a, 471; and from
(2) A. V. Burenin, E. N. Karyakin, A. F. Krupnov, S. M. Shapin, and A. N. Val'dov, 1981, J. Mol. Spectrosc. 85, 1.
The 33S hyperfine split 2 – 1 transition was taken from
(3) I. Merke and H. Dreizler, 1987, Z. Naturforsch. 42a, 1043;
and the corresponding 1 – 0 transition from
(4) J.-U. Grabow and W. Stahl, 1990, Z. Naturforsch. 45a, 1043.
Predictions beyond J = 60 should be viewed with some caution.
The 17O hyperfine splitting may be resolved for lower J transitions. Therefore, a separate hyperfine calculation up to J" = 5 is provided. The 17O spin multiplicity of 6 was considered in the calculation of the partition function !
The dipole moment was estimated from
(5) K. Tanaka, T. Tanaka, and I. Suzuki 1985, J. Chem. Phys. 82, 2835.

Lines Listed99
Frequency / GHz< 1161
Max. J99
log STR0-6.5
log STR1-5.6
Isotope Corr.-3.45
Egy / (cm-1)0.0
 µa / D0.7149
 µb / D 
 µc / D 
 A / MHz 
 B / MHz5883.67
 C / MHz 
 Q(500.0)10634.0333
 Q(300.0)6379.3542
 Q(225.0)4784.4918
 Q(150.0)3189.9791
 Q(75.00)1595.8163
 Q(37.50)798.8668
 Q(18.75)400.4270
 Q(9.375)201.2199
detected in ISM/CSMno


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