The Supergiant HD 33579

Details The Supergiant HD 33579 The Supergiant HD 33579

Nov 1968

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1968ap%26ss...2..344w&link_type=abstract

Astrophysics and Space Science, Volume 2, Issue 3, pp.344-351

Astronomy and Astrophysics

Astrophysics

15

Scientific paper

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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