Transition Probabilities and Dissociation Energy of Astrophysical Molecule CRH

Details Transition Probabilities and Dissociation Energy of Astrophysical Molecule CRH Transition Probabilities and Dissociation Energy of Astrophysical Molecule CRH

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.225..271r&link_type=abstract

Astrophysics and Space Science, Volume 225, Issue 2, pp.271-274

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

The Franck-Condon (FC) factors (transition probabilities) andr-centroids have been evaluated by the reliable numerical integration procedure for the bands of the A6∑+ →X 6∑+ system of astrophysical molecule CrH, using a suitable potential. The dissociation energyD {0/0} = 2.3 eV for the electronic ground state of CrH has been estimated by fitting the Hulburt-Hirschfelder function to the experimental potential energy curve, using the correlation coefficient.

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