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Paper: |
Long-Term Variations of Hα Emission of Be Stars in NGC 330 |
Volume: |
361, Active OB-Stars: Laboratories For Stellar and Circumstellar Physics |
Page: |
437 |
Authors: |
Hummel, W. |
Abstract: |
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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