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The Analysis of Chemical Composition of Am Star Atmospheres
Published online by Cambridge University Press: 12 April 2016
Abstract
The Survey of principal physical characteristics of the atmospheres of Am stars has been carried out. The anomalies of chemical composition have been discussed. The deficiency in C, O, Mg, Ca, and Sc alongside the excesses of heavier-than-Ni elements, with respect to Fe has been pointed out. The hypothesis on the nature of the observed anomalies are briefly discussed.
- Type
- Section IV - Non-Magnetic CP and Related Stars
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- Copyright
- Copyright © Reidel 1986