Long-Term Variations of Hα Emission of Be Stars in NGC 330

Details Long-Term Variations of Hα Emission of Be Stars in NGC 330 Long-Term Variations of Hα Emission of Be Stars in NGC 330

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..437h&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

Scientific paper

We perform an observational test on the predicted dependence of V/R
cycle times of Be stars on metallicity. Our observed Hα line
profiles variations of Be stars in the metal-deficient environment of
the SMC and the comparison to their galactic counterparts indicate that
V/R cycle times are not dependent on metallicity.

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