An evolved post-main sequence supergiant that has been observed in a S Doradus type outburst. In quiescence an LBV may have the following qualities resembling and B or Of-type supergiant:
- Hydrogen emission.
- Some have He I emission.
- Most show Fe II emission with some having [Fe II] emission.
- Free-free emission in the near-infrared but NO warm dust.
A star that has the spectroscopic characteristics of a classical LBV but has never been observed in an S Doradus type outburst is properly classified as a Candidate LBV.
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| LGGS | Name | Class | Last Measured V_mag | Table | Graph | Variability | |
|---|---|---|---|---|---|---|---|
 | J004302.52+414912.4 | AE And | LBV | 17.31 | Table | Graph | Variability |
 | J004333.09+411210.4 | AF And | LBV | 15.97 | Table | Graph | Variability |
 | J004419.43+412247.0 | Var 15 | LBV | 16.96 | Table | Graph | Variability |
 | J004450.54+413037.7 | Var A1 | LBV | 16.95 | Table | Graph | Variability |
 | J004526.62+415006.3 | M31-004526.62 | LBV | 16.88 | Table | Graph | Variability |
 | J013312.81+303012.6 | M33C-4119 | LBV | 17.69 | Table | Graph | Variability |
 | J013335.14+303600.4 | Var C | LBV | 16.16 | Table | Graph | Variability |
 | J013349.23+303809.1 | Var B | LBV | 17.31 | Table | Graph | Variability |
 | J013410.93+303437.6 | Var 83 | LBV | 16.76 | Table | Graph | Variability |
 | J013418.37+303837.0 | Var 2 | LBV | 18.11 | 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