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A spectroscopic study of Be-like variable stars in the Small Magellanic Cloud
Published online by Cambridge University Press: 12 July 2011
Abstract
Photometric searches for Be stars in environments with different metallicities have led to the discovery of many Be-like star variables. The knowledge of these types of variables is still fragmentary. This work presents the preliminary results of analyzing FLAMES+GIRAFFE spectra of a sample of these Be-like stars that we have found in the Small Magellanic Cloud (SMC).
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- Copyright © International Astronomical Union 2011