2004
DOI: 10.1081/asr-120030906
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Pulsed Nozzle Fourier Transform Microwave Spectrometer: Advances and Applications

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Cited by 38 publications
(37 citation statements)
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“…On the other hand, C 6 H 5 D has a small observable dipole moment and its rotational spectrum has been observed [23]. It has a C constant (2749.7 MHz) which is also close to the A rotational constant (2765.5 MHz) of the corresponding water dimers, C 6 H 5 D-H 2 O/C 6 H 5 D-D 2 O [6,20]. Thus, a direct determination of C rotational constants of mono-substituted benzene isotopomers is possible from the data given here.…”
Section: Resultsmentioning
confidence: 91%
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“…On the other hand, C 6 H 5 D has a small observable dipole moment and its rotational spectrum has been observed [23]. It has a C constant (2749.7 MHz) which is also close to the A rotational constant (2765.5 MHz) of the corresponding water dimers, C 6 H 5 D-H 2 O/C 6 H 5 D-D 2 O [6,20]. Thus, a direct determination of C rotational constants of mono-substituted benzene isotopomers is possible from the data given here.…”
Section: Resultsmentioning
confidence: 91%
“…Thus, a direct determination of C rotational constants of mono-substituted benzene isotopomers is possible from the data given here. In these complexes, water acts as an electrophore [20] for the determination of rotational constants of 13 CC 5 H 6 and C 6 H 5 D.…”
Section: Resultsmentioning
confidence: 99%
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“…Though IR and NMR spectroscopy offer direct experimental criteria indicating the formation of hydrogen bonds, spectroscopy in every region of the electromagnetic spectrum has contributed to the growing knowledge of the hydrogen bond phenomenon. Microwave spectroscopy in a supersonic beam has provided a wealth of structural information of isolated hydrogen-bonded complexes [134,135]. Moreover, in complexes containing a quadrupolar nuclei, such as 14 N or 35 Cl, the quadrupolar coupling constants can change due to the distortion of electronic environment around these atoms, following hydrogen bond formation [77,136].…”
Section: Spectroscopic Evidencementioning
confidence: 99%
“…This has aided the successful astronomical observation of some of these linear carbon chain species. However, the fact that some of the experimental conditions; precise dilution factor, the right choices for the precursor and inert gases, parameters of the electrical discharge source cannot be specifically controlled has made the approach 'hit or miss' as one can only probe what is produced from the source but cannot specifically control what is produced (McCarthy et al, 1997Thaddeus et al, 1998;Arunan et al, 2004). As a result, a number of species like the ions that are known not only to be present and detectable in ISM but also to be playing important role in the formation processes of other molecules in space cannot be detected because of the lack of accurate spectroscopic parameters.…”
Section: Introductionmentioning
confidence: 99%