Table 4
Massive stars with spectral type, within the selected distance range, for each of the four regions.
| WISE/Sharples/MWSC | SIMBAD id | 2MASS id | ST | STa | E(B−V) | Vo − Mv | SP–dist | Gaia–dist |
|---|---|---|---|---|---|---|---|---|
| (mag) | (kpc) | |||||||
| Sh 2–177 | ||||||||
| BD+61 105 | 00311918+6225393 | O9 Ve | O9.0 V | 0.6 | 11.7 | 2.2 | 2.7 ± 0.1 | |
| DP65 15 | 00321031+6239291 | B3–4 Ve | B3.0 V | 0.8 | 12.9 | 3.8 | 3.8 ± 0.2 | |
| G119.437–00.916 2 Mayer 1 | ||||||||
| BD+60 39 | 00215389+6145026 | O9 V | O9.0 V | 0.6 | 11.9 | 2.4 |  |
|
| LS I +61 142 | 00220494+6133577 | B0.5 V | B0.5 V | 0.6 | 12.2 | 2.8 |  |
|
| LS I +61 137 | 00212714+6144129 | B0.5 V | B0.5 V | 0.9 | 12.3 | 2.9 | 2.9 ± 0.1 | |
| LS I +61 145 | 00222651+6149398 | B1 V | B1.0V | 0.5 | 12.9 | 3.8 | 2.8 ± 0.1 | |
| LS I +61 143 | 00221278+6144405 | B2 V | B2.0 V | 0.5 | 13.3 | 4.5 | 2.6 ± 0.1 | |
| G123.155–06.306 – Sh 2–184 – IC1590 | ||||||||
| NAME HD 5005AB | 00524924+5637394 | O4 V+O9.7 II–III | O4.0V | 0.5 | 12.4 | 3.0 | 3.0 ± 0.2 | |
| HD 5005C | 00524947+5637369 | O8.5 V(n) | O8.5 V | 0.5 | 12.3 | 2.9 | 2.7 ± 0.2 | |
| HD 5005D | 00524895+5637308 | O9.2 V | O9.5 V | 0.5 | 12.5 | 3.2 | 2.5 ± 0.1 | |
| Cl IC 1590 GT 65 | 00524895+5639084 | B1.5 Vn | B1.5 V | 0.4 | 12.4 | 3.0 | 2.9 ± 0.2 | |
| GSC 03663–01289 | 00523631+5636001 | B1.5 V | B1.5 V | 0.5 | 12.2 | 2.8 |  |
|
| Cl IC 1590 GT 194 | 00520056+5636064 | B1.5 Vn | B1.5 V | 0.7 | 12.4 | 3.0 | 2.9 ± 0.2 | |
| LS I +56 10 | 00521526+5639080 | B2 Vn | B2.0 V | 0.4 | 12.5 | 3.2 |  |
|
| HD 5005E | 00524835+5637535 | B2.5 Vnn | B2.5 V | 0.5 | 13.3 | 4.6 | 2.4 ± 0.1 | |
| LS I +56 12 | 00524439+5637043 | B2.5 Vne | B2.5 V | 0.4 | 11.9 | 2.4 | 2.7 ± 0.2 | |
| Cl IC 1590 GT 213 | 00524336+5637113 | B3 Vn | B3.0 V | 0.4 | 12.5 | 3.2 |  |
|
| Cl IC 1590 GT 93 | 00531259+5638371 | B3 V | B3.0 V | 0.4 | 12.9 | 3.8 |  |
|
| Cl IC 1590 GT 95 | 00531652+5638323 | B6 V | B6.0 V | 0.4 | 12.1 | 2.6 | 2.5 ± 0.1 | |
| Cl IC 1590 GT 215 | 00525113+5636560 | B8 Ve | B8.0 V | 0.6 | 11.7 | 2.2 | 2.7 ± 0.1 | |
| Cl IC 1590 GT 150 | 00525212+5638014 | B8 V | B8.0 V | 0.4 | 12.3 | 2.9 | 2.6 ± 0.1 | |
| Cl IC 1590 GT 151 | 00524555+5637544 | B8 V | B8.0 V | 0.5 | 12.5 | 3.2 | 2.8 ± 0.1 | |
| G123.836–01.762 | ||||||||
| BSD 8–952 | 00595871+6057517 | B7 V | B7.0 V | 0.8 | 12.7 | 3.5 |  |
|
Notes. We listed the main parameters of stars with LC V used in the spectrophotometric determination The successive columns indicate: the SIMBAD and 2MASS source name, its ST, the ST adopted for the calculations, the calculated E(B−V) and distance module, the spectrophotometric distance, and the geometric distance determined by Bailer-Jones et al (2021)
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