$^{1.}$ J. I. Duncan, I. J. Wright, and D. Ellis, J. Mol. Spectrosc. 37, 394 (1971). $^{2.}$ T. Al Adlounl, F. Meyer, G. Meyer .J.G. Layabe. and A. Fayt, Int .J. Infrared and Millimeter Waves 7, 405 (1986). $^{3.}$ R. K. Thomas and H. W. Thompson, Spectrochim. Acta. 24A. 1353 (1968).Author Institution: Molecular Physics Division, National Institute of Standards and Technology; Spectroscopy Division, Bhabha Atomic Research CentreMethyl acetylene (propyne) is of interest because of its presence in planetary atmospheres, application in optically pumped lasers, and possible sotope enrichment. Almost all the energy levels of the isotopic propynes interact strongly giving a variety of perturbation effects, which make their vibration-rotation spec...
Author Institution: Department of Chemistry, Princeton UniversityBy sequentially exciting the acetyl...
This is the first report in a project to record high resolution IR data of the $^{13}$C and D substi...
\begin{wrapfigure}{l}{0pt} \includegraphics[scale=0.2]{C3D8.eps} \end{wrapfigure} We are continuing ...
$^{1.}$ J. I. Duncan, I. J. Wright, and D. Ellis, J. Mol. Spectrosc. 37, 394 (1971). $^{2.}$ T. Al A...
Propyne (CH$_{3}$-C$\equiv$CH) is an important molecule in astrophysics and planetary atmospheres, a...
In the past few decades, many high-resolution spectroscopic studies have been dedicated to the C-H s...
Author Institution: Laboratoire de Spectroscopie Hertzienne (URA CNRS), Universite de Lille I.; Facu...
The acetylenic CH stretch ($\nub{1}$) fundamental band of propyne is known to have a "double-crossin...
The aim of this work is the study of the spectrum of propyne ( CH3CCH ) in the range 6200-6700 cm-1....
The absorption spectrum of propyne (CH3CCH) has been investigated in the range 6200-6700 cm (1). Dat...
Author Institution: Department of Chemistry, University of RochesterDirect absorption of an F-center...
$^{1}$ This work supported by Grant \#B-842 The Robert A. Welch Foundation, Houston, TX.Author Insti...
Author Institution: Joint Institute for Laboratory Astrophysics, University of Colorado and National...
The results of ab initio calculations at the MP2 level of theory are presented, which provide refine...
This is a further report in a project to record high resolution IR data of the $^{13}$C and D substi...
Author Institution: Department of Chemistry, Princeton UniversityBy sequentially exciting the acetyl...
This is the first report in a project to record high resolution IR data of the $^{13}$C and D substi...
\begin{wrapfigure}{l}{0pt} \includegraphics[scale=0.2]{C3D8.eps} \end{wrapfigure} We are continuing ...
$^{1.}$ J. I. Duncan, I. J. Wright, and D. Ellis, J. Mol. Spectrosc. 37, 394 (1971). $^{2.}$ T. Al A...
Propyne (CH$_{3}$-C$\equiv$CH) is an important molecule in astrophysics and planetary atmospheres, a...
In the past few decades, many high-resolution spectroscopic studies have been dedicated to the C-H s...
Author Institution: Laboratoire de Spectroscopie Hertzienne (URA CNRS), Universite de Lille I.; Facu...
The acetylenic CH stretch ($\nub{1}$) fundamental band of propyne is known to have a "double-crossin...
The aim of this work is the study of the spectrum of propyne ( CH3CCH ) in the range 6200-6700 cm-1....
The absorption spectrum of propyne (CH3CCH) has been investigated in the range 6200-6700 cm (1). Dat...
Author Institution: Department of Chemistry, University of RochesterDirect absorption of an F-center...
$^{1}$ This work supported by Grant \#B-842 The Robert A. Welch Foundation, Houston, TX.Author Insti...
Author Institution: Joint Institute for Laboratory Astrophysics, University of Colorado and National...
The results of ab initio calculations at the MP2 level of theory are presented, which provide refine...
This is a further report in a project to record high resolution IR data of the $^{13}$C and D substi...
Author Institution: Department of Chemistry, Princeton UniversityBy sequentially exciting the acetyl...
This is the first report in a project to record high resolution IR data of the $^{13}$C and D substi...
\begin{wrapfigure}{l}{0pt} \includegraphics[scale=0.2]{C3D8.eps} \end{wrapfigure} We are continuing ...