Hönl-London factors for systems - numerical results

Details Hönl-London factors for systems - numerical results Hönl-London factors for systems - numerical results

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010mnras.402.1339t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 402, Issue 2, pp. 1339-1341.

Astronomy and Astrophysics

Astronomy

Molecular Data

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Hönl-London factors for systems - numerical results does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Hönl-London factors for systems - numerical results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hönl-London factors for systems - numerical results will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1097493