Experimental determination of the band oscillator strengths fill of the CO A(1) Pi (11<=v'<=23)-X(1}Sigma ({+)) (v''=0) made fill at the LURE-SuperACO synchrotron facility.

Details Experimental determination of the band oscillator strengths fill of the CO A(1) Pi (11<=v'<=23)-X(1}Sigma ({+)) (v''=0) made fill at the LURE-SuperACO synchrotron facility. Experimental determination of the band oscillator strengths fill of the CO A(1) Pi (11<=v'<=23)-X(1}Sigma ({+)) (v''=0) made fill at the LURE-SuperACO synchrotron facility.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...346..705e&link_type=abstract

Astronomy and Astrophysics, v.346, p.705-712 (1999)

Astronomy and Astrophysics

Astrophysics

23

Molecular Data, Ism: Molecules, Ultraviolet: Ism

Scientific paper

The band-integrated absorption oscillator strengths of the CO A(1) Pi (11<=v'<=23)-X(1}Sigma ({+)) (v''=0) transition have been measured using monochromatized synchrotron radiation from the LURE-SuperACO facility as background source. The absorption spectra were analyzed using the simulation-fitting technique described in an earlier publication (Jolly et al. 1997). Up to v'=20, the results are in good agreement with very recent ab initio calculations (Spielfiedel et al. 1999) and VUV laser measurements( Stark et al. 1998). For v'=23 which is measured here for the first time, and for v'=21 the measured oscillator strengths are found to be significantly larger than the calculated ones. Combining experimental and calculated results, a set of recommended oscillator strengths is proposed.

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