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| 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.
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