ROTATIONAL SPECTRA OF ALL O-17-BISUBSTITUTED OZONES - COMPARISON BETWEEN DIFFERENT STRUCTURES

被引:12
作者
COLMONT, JM
DEMAISON, J
COSLEOU, J
机构
[1] Laboratoire de Spectroscopie Hertzienne, URA CNRS 249, Université de Lille I, 59655 Villeneuve D’Ascq Cedex
关键词
D O I
10.1006/jmsp.1995.1132
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
We report here the results of a millimeter-wave study of all four possible bi-O-17 isotopic species of ozone, carried out in the frequency range from 49 to 393 GHz. Using Watson's Hamiltonian expressed in the A-reduction form, the rotational constants and centrifugal distortion coefficients up to the sextic terms are accurately determined for each form. The structures calculated by different procedures are compared. (C) 1995 Academic Press, Inc.
引用
收藏
页码:453 / 467
页数:15
相关论文
共 35 条
[1]  
Colmont J.M., Drean P., J. Mol. Spectrosc., 169, pp. 190-200, (1995)
[2]  
Depannemaeker J.C., Bellet J., J. Mol. Spectrosc., 66, pp. 106-120
[3]  
Tanaka T., Morino Y., J Mol. Spectrosc., 33, pp. 538-551
[4]  
Cohen E.A., Pickett H.M., J. Mol. Struct., 97, pp. 97-100, (1983)
[5]  
Rinsland C.P., Smith M.A.H., Malathy Devi V., Perrin A., Flaud J.M., Camy-Peyret C., J. Mol. Spectrosc., 149, pp. 474-480, (1991)
[6]  
Heyart M., Perrin A., Flaud J.M., Camy-Peyret C., Rinsland C.P.M.A., Smith H., Malathy Devi V., J. Mol. Spectrosc., 156, pp. 210-216, (1992)
[7]  
Heyart M., Flaud J.M., Camy-Peyret C., Rinsland C.P., Smith M.A.H., Malathy Devi V., J. Mol. Spectrosc., 157, pp. 524-531
[8]  
Colmont J.M., J Mol. Spectrosc., 168, pp. 621-623
[9]  
Consalvo D., Perrin A., Flaud J.M., Camy-Peyret C., Valentin A., Chardonnet C.H., J. Mol. Spectrosc., 168, pp. 92-98, (1994)
[10]  
Griggs M., J. Chem. Phys., 49, pp. 2-5, (1968)