Issue |
Astron. Astrophys. Suppl. Ser.
Volume 117, Number 3, June II 1996
|
|
---|---|---|
Page(s) | 561 - 568 | |
DOI | https://doi.org/10.1051/aas:1996174 | |
Published online | 15 June 1996 |
Analytic representations of rovibrational dipole matrix elements for the CO molecule and its isotopomers
DAEC et URA 173 du CNRS, Observatoire de Paris-Meudon, Place Jules Janssen, F-92195 Meudon Principal, France e-mail: roueff@obspm.fr
Send offprint request to: E. Roueff
Received:
20
July
1995
Accepted:
18
December
1995
We report new calculations of transition matrix elements for
more than thirty thousand infrared lines of the CO molecule and
its isotopomers inside the X ground electronic state. These
lines belong to the
=1, 2, 3 bands involving very high excited
states such as
41 and
133. The transition matrix elements
have been calculated from an accurate solution of the
Schrödinger equation by using two different theoretical electric
dipole moment functions (Werner 1981; Langhoff & Bauschlicher
1995). For low lying levels, our data compare satisfactorily
with experimental ones and related works (Goorvitch &
Chackerian 1994a, b; Chackerian et al. 1994, Goorvitch 1994).
Moreover, we make predictions for oscillator strengths and
Einstein coefficients involving high excited transitions. In
addition, we report simple analytic formulae that fit our
results for 12C16O with an accuracy better than 10-2 as a
function of
for each vibrational
sequence and band. They offer an easy way to compute the various
intensities of these rovibrational transitions whose transition
energies may be introduced via the available Dunham
coefficients.
Key words: molecular data / ISM: molecules
© European Southern Observatory (ESO), 1996