Evaluation of astrophysically useful parameters for HD molecule

Details Evaluation of astrophysically useful parameters for HD molecule Evaluation of astrophysically useful parameters for HD molecule

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aph....26..186k&link_type=abstract

Astroparticle Physics, Volume 26, Issue 3, p. 186-189.

Physics

1

Oscillator And Band Strengths, Lifetimes, Transition Moments, And Franck-Condon Factors

Scientific paper

The spectrum of HD molecule is the testing ground of both refined calculations and experimental techniques and its excited states are of considerable relevance to chemistry and astrophysics. In this study, the Franck Condon (FC) factors and r-centroids are evaluated for the bands of d3Π a3Σg+, e 3Σu+ a3Σg+ and I 1Π B1Σu+ transitions of HD molecule. The evaluation is done by numerical integration procedure using a suitable potential. The physical and astrophysical significance of the estimated FC factors and r-centroids are also discussed.

Affiliated with

Also associated with

No associations

Rating

Evaluation of astrophysically useful parameters for HD molecule does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Evaluation of astrophysically useful parameters for HD molecule, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evaluation of astrophysically useful parameters for HD molecule will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-869293