The structure of ScC2 (X̃2A1): A combined Fourier transform microwave/millimeter-wave spectroscopic and computational study

2020 ◽  
Vol 153 (3) ◽  
pp. 034304 ◽  
Author(s):  
M. A. Burton ◽  
Q. Cheng ◽  
D. T. Halfen ◽  
J. H. Lane ◽  
N. J. DeYonker ◽  
...  
1980 ◽  
Vol 87 ◽  
pp. 631-632
Author(s):  
Donald N. B. Hall

During the past week we have heard a considerable number of papers dealing with spectroscopic observations in the 1-5μm region of the infrared. I predict that as instruments and detectors continue to improve, such observations will play a major role in the study of interstellar molecules in both molecular clouds and circumstellar clouds around evolved stars. Fourier Transform spectrometers and Fabry Perot interferometers have already yielded spectra of such sources with spectral resolution and radial velocity precision fully comparable to millimeter wave observations. The critical need is to improve the limiting magnitude of such observations by 3-5 stellar magnitudes so that one can study large numbers of sources rather than the few brightest in each class.


2018 ◽  
Vol 20 (16) ◽  
pp. 11047-11052 ◽  
Author(s):  
D. T. Halfen ◽  
L. M. Ziurys

The pure rotational spectrum of the AlC2 radical (X̃2A1) has been measured using Fourier transform microwave/millimeter-wave (FTMmmW) techniques in the frequency range 21–65 GHz.


2010 ◽  
Vol 114 (14) ◽  
pp. 4776-4784 ◽  
Author(s):  
Stéphane Bailleux ◽  
Patrik Kania ◽  
Jan Skřínský ◽  
Toshiaki Okabayashi ◽  
Mitsutoshi Tanimoto ◽  
...  

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