Vibration–rotation infrared emission spectrum of hydrogen isocyanide, HNC, at 2.75 µm

Author(s):  
Marcus J. Winter ◽  
W. Jeremy Jones
2004 ◽  
Vol 82 (6) ◽  
pp. 947-950 ◽  
Author(s):  
Alireza Shayesteh ◽  
Dominique RT Appadoo ◽  
Iouli Gordon ◽  
Peter F Bernath

The gaseous MgD2 molecule has been synthesized for the first time in an electrical discharge inside a high-temperature furnace. The high-resolution infrared emission spectrum of MgD2 was recorded with a Fourier transform spectrometer, and the antisymmetric stretching mode (v3) was detected near 1176.5 cm–1. The v3 band was rotationally analyzed, and the r0 Mg—D bond distance was determined to be 1.700 874(8) Å.Key words: gaseous MgD2, vibration-rotation emission spectrum, Mg-D bond distance.


1978 ◽  
Vol 72 (2) ◽  
pp. 189-199 ◽  
Author(s):  
C Amiot ◽  
C Effantin ◽  
J d'Incan ◽  
J Verges

2006 ◽  
Vol 240 (1) ◽  
pp. 112-119 ◽  
Author(s):  
Nikolai F. Zobov ◽  
Roman I. Ovsannikov ◽  
Sergei V. Shirin ◽  
Oleg L. Polyansky ◽  
Jonathan Tennyson ◽  
...  

1961 ◽  
Vol 34 (2) ◽  
pp. 420-431 ◽  
Author(s):  
D. E. Mann ◽  
B. A. Thrush ◽  
D. R. Lide ◽  
J. J. Ball ◽  
N. Acquista

1984 ◽  
Vol 62 (12) ◽  
pp. 1414-1419 ◽  
Author(s):  
R. J. Winkel Jr. ◽  
Sumner P. Davis ◽  
Rubén Pecyner ◽  
James W. Brault

The infrared emission spectrum of carbon monosulfide was observed as a sequence of vibration–rotation bands in the X1Σ+ state, with strong heads of the Δν = 2 sequence degraded to the red. Eight bands of 12C32S were identified, and bands corresponding to the isotope 12C34S were also observed. The most prominent band head, that of the (2–0) band, is at 2585 cm−1, with the other heads spaced approximately 26 cm−1 to smaller wavenumbers. Our data, taken with the Fourier transform spectrometer at the National Solar Observatory (Kitt Peak) include the first reported laboratory observations of the band heads and as many as 200 lines in each band. These observations allowed the calculation of vibrational and rotational constants to higher order than previously reported.


1993 ◽  
Vol 214 (5) ◽  
pp. 527-530 ◽  
Author(s):  
Hiromichi Uehara ◽  
Koui Horiai ◽  
Yasushi Ozaki ◽  
Toichi Konno

1955 ◽  
Vol 45 (6) ◽  
pp. 455 ◽  
Author(s):  
Raymond Sloan ◽  
John H. Shaw ◽  
Dudley Williams

Science ◽  
2002 ◽  
Vol 297 (5585) ◽  
pp. 1323-1324 ◽  
Author(s):  
P. F. Bernath

1983 ◽  
Vol 98 (1) ◽  
pp. 168-184 ◽  
Author(s):  
C.M. Clayton ◽  
D.W. Merdes ◽  
J. Plíva ◽  
T.K. McCubbin ◽  
R.H. Tipping

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