Table C.2.
Stars that are probably not classical Be stars.
| Name | HD | RA | Dec | V | SpT | SpT refs | Comments |
|---|---|---|---|---|---|---|---|
| J2000 | J2000 | mag | |||||
| BD+61 105 | 00 31 19.201 | 62 25 39.442 | 9.3 | O9 IV | Negueruela et al. (2004) | ||
| BD+63 124 | 01 01 12.074 | 63 57 14.405 | 10.9 | B1Ve | Jaschek & Egret (1982) | ||
| BD+59 334 | 01 51 09.313 | 60 26 10.833 | 10.6 | B0 V | Hardorp et al. (1959) | ||
| HD 232590 | 232590 | 02 03 48.894 | 55 07 14.523 | 8.6 | B1.5IIIe | Morgan et al. (1955) | |
| V355 Per | 13758 | 02 16 04.433 | 57 44 41.674 | 9.1 | B1Ve | Jaschek & Egret (1982) | App, contact system (Avvakumova et al. 2013) |
| ... |
Notes. The first two columns give the star name and the HD number. Columns 3 and 4 give the coordinates of the target, while the next column gives the V-band magnitude. In the column “SpT” we give the most recent spectral type from literature and in “SpT Refs” the corresponding spectral type reference. Individual comments on each target are given in the “Comments” column (see notes for the abbreviations used). The abbreviation “em” stands for emission. A full version of this table is available at the CDS. The first few lines are shown as an example.
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