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Oscillator Strengths for Visible and Ultraviolet Observations of Interstellar Molecules
Published online by Cambridge University Press: 04 August 2017
Abstract
The accuracy of the information obtained from observations of optical-wavelength, molecular absorption features in interstellar clouds is directly limited by the accuracy of the rotational-line oscillator strengths used in the analysis of data. This paper briefly discusses optical observations of molecules in interstellar clouds; surveys molecular lifetime and oscillator strengths; and reviews laboratory techniques for obtaining these data.
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- Copyright © Reidel 1987