Table 3
Spectral properties and heliocentric RVs.
| Star ID | V/(B–V)(a) | MKlit.(b) | MKNOT(c) | DIB(d) | AV | V(Lit.)(e) (km s−1) | V(NOT)(f) (km s−1) | Number(g) nights | Notes(h) |
|---|---|---|---|---|---|---|---|---|---|
| V747 Cep(*) | 10.07/1.31 | O5.5 V | O5.5 V | s | 6.1 | EB, SB 1 | 12 | br | |
| BD+66° 1675 | 9.08/1.08 | O7.5 V | O6 V/O8 V/B | s | 4.6 | −9.91−9.32 | SB3 | 13 | |
| P16 | 11.81/1.91 v | O9 | O7 V | s | 9.4 | SB1 | 7 | ||
| IR star(**) | O9 V | s | 11.9 | SB1 | 18 | ||||
| BD+66° 1674 | 9.60/1.07 | O9.7 IV | B0 III/B | s | 3.4 | −9.11+5.22 | SB2, SB3? | 12 | |
| P66 | 12.95/1.54 | B0.5 V | s | 6.9 | −20.4±3.4 | 2 | |||
| P3 | 11.30/1.14v | B0.5 V | B0.5 V | s | 3.7 | −24.52 | −14.4±2.8 | 12 | br |
| P310 | 12.48/1.32 | B1 V(n) | s | 6.1 | −21.1 ±2.4 | ||||
| P130 | 12.61/1.63 | B1 V(n) | s | 7.6 | −22.0±4.2 | 2 | br | ||
| P23 | 13.84/1.64 | B2.5Vn | s | 6.1 | SB1 | 2 | br | ||
| P62 | 13.48/1.19 | B3 Vn | s | 4.4 | −16.2±2.2 | ||||
| P114 | 12.43/1.35 | B3 V(n) | s | 5.3 | −18.7±5.4 | 2 | br | ||
| P15 | 12.78/1.25 v | B3 V | B5 Vn | s | 5.1 | −17.5±3.4 | 2 | ||
| P13 | 13.64/1.30 | B5 Vn | s | 4.2 | −24.5±1.3 | 2 | br | ||
| P105 | 13.65/1.43 | B5 Vn | s | 6.8 | −21.2±4.6 | br | |||
| P20 | 13.40/1.43 v | B8 III | B8 Vn | s | 4.5 | −16.5±6.6 | 2 | ||
| P59 | 14.88/1.42 | B9 Vn | s | 4.6 | −21.8±5.8 | ||||
| P195 | 14.22/1.47 | B9 Vn | s | 4.1 | −14.2±9.5 | ||||
| P7 | 13.87/1.24 | A1 Vn | s | 3.9 | −15.3±1.2 | 2 | |||
| P316 | 12.47/0.72 | A5 V | w | 1.2 | −20.4±3.8 | nm | |||
| P233 | 13.00/0.82 | F8 IVn | w | 0.3 | −12.0±0.9 | nm | |||
| P164 | 12.27/0.60 | G2 V | n | 0.3 | −6.0±0.2 | nm | |||
| P239 | 12.95/1.03 | G3 V | w | 0.5 | −30.0±1.0 | nm | |||
| P121 | 13.42/0.85 v | G5 Vn | n | 1.1 | −7.2±0.3 | nm | |||
| P201 | 12.43/0.86 v | G5 V | n | 0.6 | −50.33 | SB2 | nm | ||
| P109 | 13.50/1.12 v | G8 Vn | w | 1.0 | −29.23 | −30.5±0.7 | nm | ||
| P106 | 14.32/1.19 v | K5 Vn | n | 0.0 | −12.9±1.5 | nm |
Notes. (*)BD+66° 1673. (**)2MASS J00012663+6723461. (a)Photometric data from Pandey et al. (2008) except for BD+66° 1673, 1674, 1675 taken from Majaess et al. (2008); stars marked v: variable in brightness according to Lata et al. (2011) and/or as listed in SIMBAD. (b)Spectral class from SIMBAD.(c)Spectral class from NOT spectra. Components in binaries are separated.(d)Diffuse interstellar bands: strong (s), weak (w), or not present (n) (e)Heliocentric RV from the literature: 1. Crampton & Fisher (1974); 2. Liu et al. (1989); 3. Gaia Data Release no 2. (f)Heliocentric RV derived from NOT spectra; close binaries are noted as single-lined S B1, double-lined S B2, triple-lined SB3, and eclipsing binary EB. (g)Number of nights of observations if more than one. (h)br: broad lines with v sin i:s > 150 km s−1; nm: not member.
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