INFRARED-ABSORPTION AND EMISSION-SPECTRA OF SIO

被引:37
作者
CAMPBELL, JM
KLAPSTEIN, D
DULICK, M
BERNATH, PF
机构
[1] UNIV WATERLOO,CTR MOLEC BEAMS & LASER CHEM,DEPT CHEM,WATERLOO,ON N2L 3G1,CANADA
[2] KITT PEAK NATL OBSERV,NATL OPT ASTRON OBSERV,TUCSON,AZ 85726
关键词
LINE; IDENTIFICATION; MOLECULAR DATA;
D O I
10.1086/192238
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High-resolution Fourier transform infrared spectra of SiO were recorded from two sources, the umbral region of a sunspot and a high-temperature laboratory cell. Rovibrational transitions in the sunspot absorption spectrum were measured in consecutive vibrational bands from (1, 0) to (13, 12) with J values as high as 141 for (SiO)-Si-28-O-16 (1258 lines) and (1, 0) to (6, 5) for (SiO)-Si-29-O-16 and (SiO)-Si-30-O-16 (455 lines). In the lower temperature laboratory emission spectrum only 387 rotational lines in the (1, 0) to (5, 4) bands were measured exclusively for (SiO)-Si-28-O-16. The laboratory spectrum served primarily to calibrate the lines in the sunspot spectrum to absolute rest frequencies. An improved set of Dunham constants for the (1) Sigma(+) ground state was obtained from a global fit of a combined data set consisting of our IR data and all the previously reported microwave and millimeter-wave data. In addition, an internuclear potential for the (1) Sigma(+) ground state, in the form of a parameterized modified-Morse function, was also obtained by fitting the data directly to the eigenvalues of the radial Schrodinger equation.
引用
收藏
页码:237 / 254
页数:18
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