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High Signal to Noise Analysis of the Chemical Composition of Stars in the Magellanic Clouds
Published online by Cambridge University Press: 19 July 2016
Abstract
A few high S/N spectra of F-G supergiants in the field of the Magellanic Clouds, and a spectrum of a star in the in the young SMC cluster NGC330 have been obtained at the échelle spectrograph of the 3.6m telescope of ESO (CASPEC). Preliminary results of the analysis of these stars and their consequences in the evolution of the clouds are presented here.
- Type
- VI. Chemical Composition of Stars
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- Copyright © Kluwer 1988