Stars with B-type spectra with few absorption lines and emission lines of [O I] and [Fe II] in their spectra. Some also have [Ca II] emission lines. Most show evidence for warm circumstellar dust in their spectra.
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| LGGS | Name | Class | Last Measured V_mag | Table | Graph | Variability | |
|---|---|---|---|---|---|---|---|
 | J004043.10+410846.0 | M31-004043.10 | B[e]sg | 18.50 | Table | Graph | Variability |
 | J004057.03+405238.6 | M31-004057.03 | B[e]sg | 19.03 | Table | Graph | Variability |
 | J004220.31+405123.2 | M31-004220.31 | B[e]sg | 18.75 | Table | Graph | Variability |
 | J004221.78+410013.4 | M31-004221.78 | B[e]sg | 19.25 | Table | Graph | Variability |
 | J004229.87+410551.8 | M31-004229.87 | B[e]sg | 17.75 | Table | Graph | Variability |
 | J004320.97+414039.6 | M31-004320.97 | B[e]sg | 19.20 | Table | Graph | Variability |
 | J004415.00+420156.2 | M31-004415.00 | B[e]sg | 18.22 | Table | Graph | Variability |
 | J004417.10+411928.0 | M31-004417.10 | B[e]sg | 17.06 | Table | Graph | Variability |
 | J004442.28+415823.1 | M31-004442.28 | B[e]sg | 19.78 | Table | Graph | Variability |
 | J013242.26+302114.1 | M33-013242.26 | B[e]sg | 18.20 | Table | Graph | Variability |
 | J013324.62+302328.4 | M33-013324.62 | B[e]sg | 19.52 | Table | Graph | Variability |
 | J013333.22+303343.4 | M33C-7256 | B[e]sg | 18.79 | Table | Graph | Variability |
 | J013342.78+303256.3 | V-073722 | B[e]sg | 17.80 | Table | Graph | Variability |
 | J013349.28+305250.2 | M33C-24812 | B[e]sg | 19.04 | Table | Graph | Variability |
 | J013350.12+304126.6 | M33C-15731 | B[e]sg | 16.59 | Table | Graph | Variability |
 | J013426.11+303424.7 | M33-013426.11 | B[e]sg | 19.08 | Table | Graph | Variability |
 | J013459.47+303701.9 | M33-013459.47 | B[e]sg | 18.43 | Table | Graph | Variability |
 | J013500.30+304150.9 | M33-013500.30 | B[e]sg | 19.24 | Table | Graph | Variability |
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2023-08-14 14:15:12 UT-5