Microwave Spectra of Molecules of Astrophysical Interest VI. Carbonyl Sulfide and Hydrogen Cyanide
Microwave Spectra of Molecules of Astrophysical Interest VI. Carbonyl Sulfide and Hydrogen Cyanide
复制标题
天体物理分子的微波光谱 VI。
DOI：
10.1063/1.3253139
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发表时间：
1974
影响因子：
4.3
通讯作者：
A. Maki
中科院分区：
文献类型：
--
作者：
A. Maki
所有可用的数据上的微波光谱的硫化羰和氰化氢进行了严格审查和制表。分子数据，如旋转常数，离心畸变常数，偶极矩，超精细耦合常数，结构参数也制成表格。所有的旋转过渡从100兆赫到300千兆赫，被认为是可能感兴趣的射电天文学家计算和制表沿着与他们的估计百分之九十五的置信限。微波测量列表中的大多数同位素物种和许多较低的振动状态。对于硫化羰和氰化氢的参考书目，其中包括几乎所有的光谱文献中报道的工作。对于每一个分子的相关天体物理论文的参考书目也给出了。
All available data on the microwave spectra of carbonyl sulfide and hydrogen cyanide are critically reviewed and tabulated. Molecular data such as rotational constants, centrifugal distortion constants, dipole moments, hyperfine coupling constants, and structural parameters are also tabulated. All rotational transitions from 100 MHz to 300 GHz that are deemed likely to be of interest to radio astronomers are calculated and tabulated along with their estimated 95 percent confidence limits. Microwave measurements are tabulated for most isotopic species and for many of the lower vibrational states. For both carbonyl sulfide and hydrogen cyanide a bibliography is given which includes nearly all the spectroscopic work reported in the literature. For each molecule a bibliography of related astrophysical papers is also given.