1990
DOI: 10.1016/0009-2614(90)85314-3
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Carbon and oxygen K-edge photoionization of the CO molecule

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Cited by 191 publications
(130 citation statements)
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“…The polarization dependence of the absorption is depicted in Fig. 3 by the dashed curves, and, upon closer inspection of the carbon spectrum, it is clear that our results support the identification of a 3pσ progression under the 3pπ one (as suggested by Domke [45]). Also in the carbon spectrum, the polarization dependence clearly reveals the 3dπ shoulder to the left of the 4pπ band, and, for oxygen, we note the 4sσ shoulder (relevant polarization is plotted in red (lighter gray)) to the left of the 3dπ/4pπ bands.…”
Section: Carbon Monoxidesupporting
confidence: 72%
“…The polarization dependence of the absorption is depicted in Fig. 3 by the dashed curves, and, upon closer inspection of the carbon spectrum, it is clear that our results support the identification of a 3pσ progression under the 3pπ one (as suggested by Domke [45]). Also in the carbon spectrum, the polarization dependence clearly reveals the 3dπ shoulder to the left of the 4pπ band, and, for oxygen, we note the 4sσ shoulder (relevant polarization is plotted in red (lighter gray)) to the left of the 3dπ/4pπ bands.…”
Section: Carbon Monoxidesupporting
confidence: 72%
“…As it follows from the data in Figures 2,3, the swap from scheme (b) (series of the excited states mσ -1 nσ; n>f) to scheme (a) (series of the excited states mσ -1 nπ; n>f) leads to a strong orientation effect -the appearance in the long-wave spectral region of an additional giant elastic scattering resonance connected with the virtual excitation mσ-2π with the width of 0,20 eV (Tronc et al, 1980), the oscillator strength of 0,232 and the energy of 402,1 eV (this work) for the N 2 , and with the width of 0,16 eV (Domke et al, 1990), the oscillator strength of 0,118 and the energy of 296,1 eV (this work) for the CO molecule. …”
Section: Figurementioning
confidence: 75%
“…The presence of molecular CO on the surface gives rise to the absorption peak at 534 eV, corresponding to the O1s → 2π* orbital transition. 32 The intensity of this peak decreased with time within minutes (spectra 2′b and 3′b collected after 5 min and 2′c after 10 min), indicating that CO does not stay molecularly adsorbed on the surface at 250°C due to dissociation and reaction to produce H 2 O and CH x . The broad signal from 536 to 542 eV, present in all the conditions investigated, is reminiscent of adsorbed molecular water 33 and hydroxyl species, in agreement with the AP-XPS observations and the DRIFTS observations.…”
Section: Resultsmentioning
confidence: 99%