Author:
Féménias J.-L.,Goure J. P.,Stringat R.
Abstract
Previous work on the theoretical study of the intensity distribution in the emission spectrum of ScO is now extended and a comparison is made with some experimental spectrometric data, and some physical results such as the temperature of emission and the 'spin allowed' property of the A2Π → X2Σ transition are given and discussed. The great influence of the slight spin decoupling of the A2Π (case (a)) state on the intensity distribution is shown and is explained theoretically using the mixing coefficients obtained in a former rotational study of the spectrum.
Publisher
Canadian Science Publishing
Subject
General Physics and Astronomy
Cited by
5 articles.
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