Issue |
A&A
Volume 421, Number 1, July I 2004
|
|
---|---|---|
Page(s) | 381 - 386 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361:20035871 | |
Published online | 11 June 2004 |
Effect of non-adiabatic coupling on the isotopic dependence of the photodissociation cross section of CO
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
Corresponding author: R. McCarroll, mccarrol@ccr.jussieu.fr
Received:
16
December
2003
Accepted:
15
March
2004
Calculations of the photodissociation cross sections of CO
from the ground X state into the coupled Rydberg B
state and the valence dissociative D
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
© ESO, 2004
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