1971
DOI: 10.1016/0022-2852(71)90018-x
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High resolution infrared spectrum of HCNO: Analysis of the bands at 3300 cm−1

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Cited by 23 publications
(2 citation statements)
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“…The structure and properties of HCNO such as vibrational frequencies, ionization energy, heat of formation, and so on have long been reported based on both experimental and theoretical methods. [11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26][27][28] The geometry of the HCNO has been determined by Beck et al [11][12][13] from the IR spectrum when they isolated HCNO for the first time in the pure state. Their results show that this acid has three bonds including H─C, C─N, and N─O in the molecule supporting the formyl nitrile oxide structure, HCNO, rather than the oxime structure, CNOH, 28 as proposed before.…”
Section: Introductionmentioning
confidence: 99%
“…The structure and properties of HCNO such as vibrational frequencies, ionization energy, heat of formation, and so on have long been reported based on both experimental and theoretical methods. [11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26][27][28] The geometry of the HCNO has been determined by Beck et al [11][12][13] from the IR spectrum when they isolated HCNO for the first time in the pure state. Their results show that this acid has three bonds including H─C, C─N, and N─O in the molecule supporting the formyl nitrile oxide structure, HCNO, rather than the oxime structure, CNOH, 28 as proposed before.…”
Section: Introductionmentioning
confidence: 99%
“…FTIR (the building up a spatial interferogram when a broad band frequency signal being transmitted through a sample, is scanned by translating the reference arm mirror of the interferometer through a path length that determines the spectral resolution; a Fourier transform reveals the spectrum of the transmitted signal) was later to become a major research tool for the Winnewissers. Three papers resulted from this apprenticeship using Rao's large grating spectrometers, not surprisingly about rotationally resolved mid-IR bands of HSSH and HCNO [22]- [24] Meanwhile Manfred, and Brenda upon her return, continued work on HCNO. This short "six weeks project to get the structure of HCNO", back in Karlsruhe, became the seed of a career-long program, when its rapidly apparent spectral anomalies turned out to be due to quasi-linearity, a concept not yet fully formulated at the time.…”
mentioning
confidence: 99%