The Raman spectra of gaseous, liquid and solid, and infrared spectra of gaseous and solid isopropylamine-d sub 0 and -d sub 2 was investigated between 4000 and 50 cm superscript -1. Differences between the spectrum of the solid phase and that of the fluid phases were interpreted in terms of an equilibrium between low energy s-trans and high energy gauche conformers, and a complete vibrational assignment was proposed for the s-trans conformer. The far infrared spectra of the gaseous compounds contained bands due to the asymmetric amino and coupled methyl torsions; the assignment of these bands was aided by observation of a number of two quantum transitions for each vibrational mode. The asymmetric potential functions were calculated, which r...
One of the fundamental limiting factors in ro-vibrational spectroscopy has been the lack of high bri...
International audienceThis book describes different theoretical models developed to identify the nea...
Over the last several years, our group has been involved in developing approaches to compute highly ...
The vibrational spectra from 4000 to 33 cm-1 of several modecules which may be present in the atmosp...
Infrared spectra of molecules and materials of astrophysical interest Quarterly progress report, 15...
The infrared (3500 to 40 cm-l) and Raman (3200 to 20 cm") spectra have been recorded for gaseous and...
International audienceThis book is dedicated to the description and application of various different...
Context. In the near future, high spatial and spectral infrared (IR) data of star-forming regions ob...
This thesis involves use of the Terahertz & Far-Infrared Beamline facility at the Australian Synchro...
Author Institution: CSIC, IEM. Dpt. Molecular Physics.The observation of the rotational emission of ...
Context. Infrared spectroscopy of star and planet forming regions is at the dawn of a new age with t...
Context. In the near future, high spatial and spectral infrared (IR) data of star-forming regions ob...
Author Institution: Department of Chemistry, University of South Carolina; Mobay Chemical Corporatio...
This thesis describes the infrared and Raman spectroscopic studies on ammonia, methylamine and ethyl...
One of the fundamental limiting factors in ro-vibrational spectroscopy has been the lack of high bri...
International audienceThis book describes different theoretical models developed to identify the nea...
Over the last several years, our group has been involved in developing approaches to compute highly ...
The vibrational spectra from 4000 to 33 cm-1 of several modecules which may be present in the atmosp...
Infrared spectra of molecules and materials of astrophysical interest Quarterly progress report, 15...
The infrared (3500 to 40 cm-l) and Raman (3200 to 20 cm") spectra have been recorded for gaseous and...
International audienceThis book is dedicated to the description and application of various different...
Context. In the near future, high spatial and spectral infrared (IR) data of star-forming regions ob...
This thesis involves use of the Terahertz & Far-Infrared Beamline facility at the Australian Synchro...
Author Institution: CSIC, IEM. Dpt. Molecular Physics.The observation of the rotational emission of ...
Context. Infrared spectroscopy of star and planet forming regions is at the dawn of a new age with t...
Context. In the near future, high spatial and spectral infrared (IR) data of star-forming regions ob...
Author Institution: Department of Chemistry, University of South Carolina; Mobay Chemical Corporatio...
This thesis describes the infrared and Raman spectroscopic studies on ammonia, methylamine and ethyl...
One of the fundamental limiting factors in ro-vibrational spectroscopy has been the lack of high bri...
International audienceThis book describes different theoretical models developed to identify the nea...
Over the last several years, our group has been involved in developing approaches to compute highly ...