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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2838
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dc.contributor.authorPrithivikumaran, N-
dc.contributor.authorFernandez Gomez, M-
dc.contributor.authorLopez Gonzalez, J. J-
dc.contributor.authorBagare, S. P-
dc.contributor.authorRajamanickam, N-
dc.date.accessioned2008-07-23T09:38:48Z-
dc.date.available2008-07-23T09:38:48Z-
dc.date.issued2002-
dc.identifier.citationAstrophysics and Space Science, Vol. 280, No. 4, pp. 319 - 324en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/2838-
dc.descriptionRestricted Access-
dc.description.abstractThe Franck-Condon (FC) factors (transition probabilities) and r-centroids have been evaluated by the reliable numerical integration procedure for the bands of the A^3 φ_4 --> X^3 φ_4 system of astrophysical molecule CoH, using a suitable potential. The dissociation energy D^0_0 = 2.5 +/- 0.05 eV for the electronic ground state of CoH has been estimated by fitting Hulburt-Hirschfelder function to the experimental potential energy curve, using the correlation coefficient.en
dc.format.extent57452 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/vd2fu4lnqlx0r49t/en
dc.subjectAstrophysical Molecule CoHen
dc.subjectHulburt-Hirschfelder: Functionen
dc.subjectFranck–Condon Factorsen
dc.subjectSpectroscopic Methoden
dc.titleTransition probabilities and dissociation energy of astrophysical molecule CoHen
dc.typeArticleen
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