A spectroscopic study of Be-like variable stars in the Small Magellanic Cloud

Details A spectroscopic study of Be-like variable stars in the Small Magellanic Cloud A spectroscopic study of Be-like variable stars in the Small Magellanic Cloud

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..308s&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

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1

Stars: Early-Type, Stars: Emission-Line, Be, Stars: Variables: Other

Scientific paper

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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