1992
DOI: 10.1016/0022-2852(92)90246-k
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Collisional excitation of the Comet-Tail system of CO+ [A2Πi-X2Σ+]

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Cited by 5 publications
(1 citation statement)
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“…By contrast, only the upper electronic state A 2 Π i of the comet tail system is accessible in direct collisional excitation of CO + . 12 This latter observation is surprising in view of the fact that the potential energy curve for the X 2 Σ + state of CO + (ar r e = 1.115Å) is more closely aligned with the potential energy curve for the B 2 Σ + state (at r e = 1.169Å) than that for A 2 Π i (at r e = 1.244Å). The extra energy of excitation required to reach the B 2 Σ + state is the only reasonable explanation for its absence in the TES of CO + .…”
Section: Resultsmentioning
confidence: 98%
“…By contrast, only the upper electronic state A 2 Π i of the comet tail system is accessible in direct collisional excitation of CO + . 12 This latter observation is surprising in view of the fact that the potential energy curve for the X 2 Σ + state of CO + (ar r e = 1.115Å) is more closely aligned with the potential energy curve for the B 2 Σ + state (at r e = 1.169Å) than that for A 2 Π i (at r e = 1.244Å). The extra energy of excitation required to reach the B 2 Σ + state is the only reasonable explanation for its absence in the TES of CO + .…”
Section: Resultsmentioning
confidence: 98%