Issue |
Astron. Astrophys. Suppl. Ser.
Volume 117, Number 3, June II 1996
|
|
---|---|---|
Page(s) | 557 - 559 | |
DOI | https://doi.org/10.1051/aas:1996173 | |
Published online | 15 June 1996 |
Einstein A-coefficients for vib-rotational transitions in CO
1
Department of Physics, University of Gorakhpur, Gorakhpur 273 009, India
2
Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411 007, India
Send offprint request to: S. Chandra, School of Sciences, Indira Gandhi National Open University, New Delhi 110 068, India
Received:
18
May
1995
Accepted:
1
December
1995
Einstein A-coefficients for vib-rotational transitions in CO isotopomers, for vibrational quantum number v up to 20, rotational quantum number J up to 140, and up to 4, are calculated. The change in J is governed by the selection rules . These coefficients play an important role in astronomy, as CO is the most abundant molecule after , and has been observed in almost all the astronomical objects.
Key words: ISM: molecules / molecular data
© European Southern Observatory (ESO), 1996