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On the Influence of the Chemical Composition on the Structure and Metal Index of Stellar Atmospheres.
The Astrophysical Journal1964Vol. 140, pp. 221–221
Citations Over TimeTop 15% of 1964 papers
Abstract
A series of model stellar atmospheres, representing stars of normal and low heavy-element abundance in the spectral range F() K0, have been calculated. Characteristics of the emergent flux of the models, particularly the metal index and (v, b, y)-colors of Str6mgren's narrow-band photometric system, are discussed and compared with observations.
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