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Table 4:

Number ratios of Be to (B+Be) stars as a function of spectral type in SMC and Galaxy1.
Spectral type SMC SMC % Galaxy
  % without NGC 330 %
O8-O9e 23.8 20.8 14.3
B0e 35.2 26.3 7.6
all B0e 36.1   12.7
B1e 20.6 16.7 3.4
all B1e 27.0   7.7
B2e 15.3 13.9 4.9
all B2e 19.9   7.8
B3e 9.6 8.9 3.4
all B3e 14.0   6.8
B4e 2.9 3.0 0.0
all B4e 7.6   0.0
B5e 0.0 0.0 2.2
all B5e 1.8   9.2
B6e 0.6 0.6 0.0
all B6e 1.2   0.0
B7e 0.0 0.0 2.4
all B7e 0.0   7.2
B8e 0.0 0.0 1.2
all B8e 0.0   9.3
B9e 0.0 0.0 1.8
all B9e 0.0   11.1
A0e 2.5 2.5 0.9

1 For each range in spectral type, the fractions of definite emission-line stars and the combination of definite and candidate emission-line stars are listed.

Source LaTeX | All tables | In the text

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