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Issue A&A
Volume 421, Number 1, July I 2004
Page(s) 381 - 386
Section Atomic, molecular and nuclear data
DOI http://dx.doi.org/10.1051/0004-6361:20035871



A&A 421, 381-386 (2004)
DOI: 10.1051/0004-6361:20035871

Effect of non-adiabatic coupling on the isotopic dependence of the photodissociation cross section of CO

L. Andric1, F. Bouakline1, T. P. Grozdanov2 and R. McCarroll1

1  Laboratoire de Chimie Physique-Matière et Rayonnement (UMR 7614 du CNRS), Université Pierre et Marie Curie, 75231 Paris Cedex 05, France
2  Institute of Physics, PO Box 57, 11001-Belgrade, Serbia and Montenegro

(Received 16 December 2003 / Accepted 15 March 2004)

Abstract
Calculations of the photodissociation cross sections of CO from the ground X $^1\Sigma^+$ state into the coupled Rydberg B $^1\Sigma^+$ state and the valence dissociative D $^{'1}\Sigma^+$ state have been carried out using the smooth exterior complex scaling (SECS) method. Results are presented for all of the 6 isotopomers involving the  12C, 13C, 16O, 17O and 18O isotopes. The absorption profiles of the predissociating resonances induced by non-adiabatic coupling vary considerably from one isotopomer to another. It is confirmed that resonance widths obtained simply from a diagonalization of the complex Hamiltonian do not give a true indication of the absorption profile. A correct profile is only obtained when the sum over all resonant and non-resonant continuum states is performed. A brief discussion is given of the implications for isotopic fractionation in interstellar CO.


Key words: astrochemistry -- ISM: molecules -- molecular processes -- ultraviolet: ISM

Offprint request: R. McCarroll, mccarrol@ccr.jussieu.fr




© ESO 2004

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