1956
DOI: 10.1016/0083-6656(56)90055-1
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The quantitative chemical analysis of early-type stars

Abstract: The University of Michigan programme for the determination of the abundances of the elements in hot stars involves an observational, a theoretical, and an experimental phase. A description of the spectrum of 7 Pegasi from •3570-).3970 and the profiles of the stronger lines in the photographic region illustrate the type of observational material that is being employed in this investigation. The point of view adopted for the theoretical programme is next described. Briefly, the model atmosphere of any given star… Show more

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