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The WFI Halpha spectroscopic survey of the Magellanic Clouds: Be stars in SMC open clusters

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Academic year: 2021

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Figure

Figure 1. Absolute V magnitude vs. dereddened colour (B-V)-top or (V-I)-bottom for SMC stars of our sample
Table 1. Details and comparison of samples used in this study
Figure 2. Ratios of definite Be stars to B stars as a function of spectral type in the SMC (top), and in the MW (bottom, from McSwain & Gies 2005)
Figure 3. Distribution of Be stars with spectral type in SMC (open clusters [hatched bars]) and the MW (field [filled bars], and open clusters [dotted bars]).

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