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Interpretations of Stellar Spectra: NLTE Effects
Published online by Cambridge University Press: 30 March 2016
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To solve the system of statistical balance equations and radiative transfer equations (NLTE problem) we followed the modification of linearization method proposed by Auer and Heasley (1976) and used 20-level model of the lithium atom. The 70 radiative and all possible collisional transitions were included into the rate matrix (Pavlenko 1994).
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- II. Joint Discussions
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- Copyright © Kluwer 1995
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