Emission spectra with a high resolution Fourier transform spectrometer: CO spectra and their astrophysical importance
Emission spectra with a high resolution Fourier transform spectrometer: CO spectra and their astrophysical importance
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高分辨率傅里叶变换光谱仪的发射光谱：CO 光谱及其天体物理学重要性
DOI：
10.1016/0022-2852(74)90083-6
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发表时间：
1974
影响因子：
1.4
通讯作者：
J. Maillard
中科院分区：
文献类型：
--
作者：
A. Mantz;J. Maillard
线的位置和分子常数的报告为2-0，3-1，4-2，5-3，6-4，和7-5频带的CO在发射中观察到的。未混合线位置的绝对不确定度约为±0.0003 cm-1。使用分子常数计算高分辨率恒星、太阳黑子和激光光谱（forv≤ 7，J< 100），其范围在已发布数据的实验不确定度范围内。本研究中。
Line positions and molecular constants are reported for the 2-0, 3-1, 4-2, 5-3, 6-4, and 7-5 bands of CO observed in emission. The absolute uncertainty of unblended line positions is on the order of ±0.0003 cm−1.High resolution stellar, sunspot, and laser spectra (forv≤ 7,J< 100) are calculated to within the experimental uncertainty of the published data using the molecular constants derived in this study.