Journal Article

Hönl–London factors for systems – numerical results

J. B. Tatum

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 402, issue 2, pages 1339-1341
Published in print February 2010 | ISSN: 0035-8711
Published online February 2010 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2009.15982.x
Hönl–London factors for  systems – numerical results

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The results of numerical calculations are presented for the Hönl–London factors of 3Φ−3Δ systems. These are band systems that occur in the molecular spectra of ZrO and TiO that are familiar in S- and M-type stars. In a new result, it is shown how the strengths of possible satellite branches vary with the degree of coupling of the electron spin to the internuclear axis, and for what degree of coupling the strengths of these branches are at a maximum.

Keywords: molecular data

Journal Article.  1665 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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