1973
DOI: 10.1088/0031-8949/8/5/007
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Term Values and Molecular Parameters for CH and CH+

Abstract: Term values and molecular parameters for C H and CH+. I. Botterud, A.

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Cited by 56 publications
(13 citation statements)
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“…The main reason for the discrepancy between the data for the other systems probably lies with systematic uncertainties in determining the absorption baselines at low optical densities. Combining the results for all three transitions gives a SO coupling constant of A Π ) 21 ( 1 cm -1 (reduced by ∼11 cm -1 from the gasphase value 17 ) and an orbital reduction factor of κ ) 0.26 ( 0.03.…”
Section: Discussionmentioning
confidence: 91%
See 1 more Smart Citation
“…The main reason for the discrepancy between the data for the other systems probably lies with systematic uncertainties in determining the absorption baselines at low optical densities. Combining the results for all three transitions gives a SO coupling constant of A Π ) 21 ( 1 cm -1 (reduced by ∼11 cm -1 from the gasphase value 17 ) and an orbital reduction factor of κ ) 0.26 ( 0.03.…”
Section: Discussionmentioning
confidence: 91%
“…)] (40) determining M 1 at low temperatures in the presence of a very much larger M 0 , but the data in Figure 1 give A ∆ ) 6 ( 2 cm -1 . In contrast, A ∆ ) -1.1 ( 0.2 cm -1 for CH in the gas phase, 17 which indicates that the matrix imposes a substantial external-atom SO effect on the A 2 ∆ states. M 0 and M 1 yield no information about V ∆ , the CF splitting of the A 2 ∆ term.…”
Section: Discussionmentioning
confidence: 99%
“…Extensive spectroscopic studies have been made of the ground state 78 and the lowest three excited states [79][80][81][82][83][84][85][86][87] partly because of its importance in astrophysics and chemistry. [88][89][90][91][92][93][94] Two excited state potential curves look promising for cooling CH: C 2 S + and 2 D as both have strongly fluorescing transitions to the ground state.…”
Section: Laser Cooling Of Chmentioning
confidence: 99%
“…If a plasma is optically thin, then the photon flux I(p, q) of a transition from state p to state q is given by the expression (12) where I(p, q) is in units of photon flux per unit area per unit solid angle, n(p) is the density of the emitting species p, A(p, q) is the transition probability, and integration is over the observed depth of the plasma, c~9~…”
Section: Excited Argon Neutral Densities Estimated From Relative Linementioning
confidence: 99%