$^{*}$ These research was assisted by support from Contract Nour-656(12) NR 019-401 of the office Naval Research.Author Institution: The Pennsylvania State UniversityMore than 40 bands of the HCN molecule are available for performing the vibrational analysis. About 20 of these bands in the $1.1 \mu$ to $3.0 \mu$ region some of which have been observed for the first time, have been measured or remeasured. Q branches for most of the perpendicular bands have been resolved, allowing a precise determination of the band origins. It has been necessary to make use of the ten $Y_{ilk}$ coefficients to perform a satisfactory vibrational analysis. A number of cases of Fermi resonance have been observed. Several of these perturbations can be calculated...
$^{a}$D. T. Moore, M. Ishiguro, and R. E. Miller, J. Chem. Phys. 115, 5144 (2001) $^{b}$H. G. Kolsky...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
Author Institution: Department of Physics, The Ohio State UniversityThe objective of the studies of ...
Variation calculations of the vibration–rotation energy levels of many isotopomers of HCN are report...
This work supported by the U.S. Army Research Office, Grant DAAG29-77-G-0007.Author Institution: Dep...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
Author Institution: Department of Chemistry, Harvard University, Cambridge, MAHigh resolution radio ...
Author Institution: Department of Chemistry, Faculty of Sciences, Kyushu University,; Fukuoka, 812-8...
$^{1}$ K.R. Leopold, G.T. Fraser, F.J. Lin, D.D. Nelson, Jr., and W. Klemperer, J. Chem. Phys. 81. 4...
$^{1}$ K.R. Leopold, G.T. Fraser, F.J. Lin, D.D. Nelson, Jr., and W. Klemperer, J. Chem. Phys. 81. 4...
$^{a}$D. T. Moore, M. Ishiguro, and R. E. Miller, J. Chem. Phys. 115, 5144 (2001) $^{b}$H. G. Kolsky...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
Author Institution: Department of Physics, The Ohio State UniversityThe objective of the studies of ...
Variation calculations of the vibration–rotation energy levels of many isotopomers of HCN are report...
This work supported by the U.S. Army Research Office, Grant DAAG29-77-G-0007.Author Institution: Dep...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
Author Institution: Department of Chemistry, Harvard University, Cambridge, MAHigh resolution radio ...
Author Institution: Department of Chemistry, Faculty of Sciences, Kyushu University,; Fukuoka, 812-8...
$^{1}$ K.R. Leopold, G.T. Fraser, F.J. Lin, D.D. Nelson, Jr., and W. Klemperer, J. Chem. Phys. 81. 4...
$^{1}$ K.R. Leopold, G.T. Fraser, F.J. Lin, D.D. Nelson, Jr., and W. Klemperer, J. Chem. Phys. 81. 4...
$^{a}$D. T. Moore, M. Ishiguro, and R. E. Miller, J. Chem. Phys. 115, 5144 (2001) $^{b}$H. G. Kolsky...
HC3N is a ubiquitous molecule in interstellar environments, from external galaxies to Galactic inter...
Author Institution: Department of Physics, The Ohio State UniversityThe objective of the studies of ...