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<article xlink="http://www.w3.org/1999/xlink" dtd-version="1.0" article-type="general-sciences" lang="en"><front><journal-meta><journal-id journal-id-type="publisher">IJCRR</journal-id><journal-id journal-id-type="nlm-ta">I Journ Cur Res Re</journal-id><journal-title-group><journal-title>International Journal of Current Research and Review</journal-title><abbrev-journal-title abbrev-type="pubmed">I Journ Cur Res Re</abbrev-journal-title></journal-title-group><issn pub-type="ppub">2231-2196</issn><issn pub-type="opub">0975-5241</issn><publisher><publisher-name>Radiance Research Academy</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">2093</article-id><article-id pub-id-type="doi"/><article-id pub-id-type="doi-url"/><article-categories><subj-group subj-group-type="heading"><subject>General Sciences</subject></subj-group></article-categories><title-group><article-title>DISSOCIATION ENERGIES, FRANCK-CONDON FACTORS AND R-CENTROIDS OF THE SULPHIDES OF&#13;
METALS (LI AND NI )&#13;
</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>Balanarayana</surname><given-names>C.</given-names></name></contrib><contrib contrib-type="author"><name><surname>Reddy</surname><given-names>B.C. Venkata</given-names></name></contrib><contrib contrib-type="author"><name><surname>Reddy</surname><given-names>R.R.</given-names></name></contrib><contrib contrib-type="author"><name><surname>Chalapathi</surname><given-names>G.Venkata</given-names></name></contrib></contrib-group><volume>)</volume><issue/><fpage>190</fpage><lpage>198</lpage><permissions><copyright-statement>This article is copyright of Popeye Publishing, 2009</copyright-statement><copyright-year>2009</copyright-year><license license-type="open-access" href="http://creativecommons.org/licenses/by/4.0/"><license-p>This is an open-access article distributed under the terms of the Creative Commons Attribution (CC BY 4.0) Licence. You may share and adapt the material, but must give appropriate credit to the source, provide a link to the licence, and indicate if changes were made.</license-p></license></permissions><abstract><p>The experimental potential energy curves for the different electronic states of astrophysically important&#13;
LiS+ and NiS molecules are constructed by using Rydberg-Klein-Rees method as modified by&#13;
Vanderslice et al. The ground state dissociation energies are determined by curve fitting techniques using&#13;
the five parameters Hulburt-Hirschfelder (H-H) function. The estimated dissociation energies are&#13;
0.81__ampersandsignplusmn;0.02 and 3.56__ampersandsignplusmn;0.08 eV for LiS+, and NiS respectively. These values are in good agreement with the&#13;
values reported in the earlier literature. The r-centroids and Franck-Condon factors (FC factors) for the&#13;
bands of 3 -X3 - system of LiS+ and A3 -X3 - system for NiS, molecules have been calculated. The&#13;
Franck-Condon factors are evaluated by the approximated analytical methods of Jarmain and Fraser. The&#13;
absence of the bands of these systems is explained.&#13;
</p></abstract><kwd-group><kwd>Diatomic molecules; Dissociation energies; Franck-Condon factors; r-centriods</kwd></kwd-group></article-meta></front></article>
