The supergiant HD 33579

descriptionPublicationkeyboard_double_arrow_right Article 01 Nov 1968 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 2, pages 344-351 (issn: 0004-640X, eissn: 1572-946X,

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Authors: Gordon W. Wares; John E. Ross; Lawrence H. Aller;

doi: 10.1007/bf00650912

The supergiant HD 33579

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Abstract

The brightest star in either Magellanic cloud has been analyzed by the method of model atmospheres using observational data secured at Cerro Tololo. The results from abundance studies are in general accord with the conclusions by Przybylski. We find solar abundances for Fe, Sc, Mg, Si and, probably, Ca. The V, Cr, Si, Ti data suggest lower abundances but the evidence is not conclusive.

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University of California, Los Angeles
United States
United States Air Force Research Laboratory
United States

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