Transition probabilities and dissociation energy of astrophysical molecule CoH

dc.contributor.author	Prithivikumaran, N
dc.contributor.author	Fernandez Gomez, M
dc.contributor.author	Lopez Gonzalez, J. J
dc.contributor.author	Bagare, S. P
dc.contributor.author	Rajamanickam, N
dc.date.accessioned	2008-07-23T09:38:48Z
dc.date.available	2008-07-23T09:38:48Z
dc.date.issued	2002
dc.identifier.citation	Astrophysics and Space Science, Vol. 280, No. 4, pp. 319 - 324	en
dc.identifier.issn	0004-640X
dc.identifier.uri	http://hdl.handle.net/2248/2838
dc.description	Restricted Access
dc.description.abstract	The 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.extent	57452 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/vd2fu4lnqlx0r49t/	en
dc.subject	Astrophysical Molecule CoH	en
dc.subject	Hulburt-Hirschfelder: Function	en
dc.subject	Franck–Condon Factors	en
dc.subject	Spectroscopic Method	en
dc.title	Transition probabilities and dissociation energy of astrophysical molecule CoH	en
dc.type	Article	en