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Table B.1.

Spectroscopic OB stars sample.

Star id. (a) Type (a) RA, Dec (a) V(a) Gaia source id. π μα μδ G θ Distance (b) Vlon Vlat Vtot PA
(°, °) (mag) (mas) (mas yr−1) (mas yr−1) (mag) (arcsec) (kpc) (km s−1) (km s−1) (km s−1) (° )
1 B2 V 259.016,−36.314 15.68 5973950143220187776 0.618 ± 0.751 1.71 ± 1.32 −4.09 ± 0.90 14.467 0.38 −5.44 ±10.11 −20.02 ±32.85 20.75 ± 34.35 195.2
2 B2 V 259.018,−36.282 15.88 5973950349378625408 0.597 ± 0.053 0.14 ± 0.09 −2.08 ± 0.06 14.730 0.50 −0.32 ±0.05 −1.58 ± 0.27 1.61 ± 0.27 191.5
3 B3 259.123,−36.349 16.29 5973946569807373184 0.592 ± 0.048 −0.24 ± 0.09 −2.40 ± 0.06 15.250 0.70 −4.36 ±0.56 −0.65 ± 0.11 4.40 ± 0.57 261.5
4 B2 V 259.146,−36.460 15.17 5973933650545713536 0.517 ± 0.041 0.09 ± 0.08 −2.53 ± 0.05 14.485 1.27 −6.15 ±0.75 −5.16 ± 0.71 8.03 ± 1.03 230.0
5 B2 V 259.223,−36.323 15.53 5973936158806635264 0.556 ± 0.038 −0.15 ± 0.07 −2.39 ± 0.04 14.889 1.06 −5.02 ±0.52 −1.86 ± 0.24 5.36 ± 0.58 249.6
6 B3 Ia 259.252,−36.227 14.89 5973948730168050560 0.436 ± 0.107 −0.2 ± 0.17 −2.15 ± 0.12 13.074 0.03 −8.50 ±3.0 −2.89 ± 1.28 8.98 ± 3.25 251.2
7 B2 V 259.256,−36.367 15.99 5973935128014466688 0.519 ± 0.084 0.41 ± 0.14 −2.00 ± 0.10 14.887 0.97 −0.56 ±0.16 −4.69 ± 1.29 4.73 ± 1.3 186.8
8 B2 V 259.260,−36.335 15.66 5973936021367671168 0.202 ± 0.047 −0.2 ± 0.08 −2.91 ± 0.05 14.936 0.79 −48.85±13.1 −26.91 ±7.92 55.77 ± 15.3 241.2
9 B2 V 259.298,−36.328 16.08 5973935677770283136 0.549 ± 0.064 0.03 ± 0.11 −2.31 ± 0.07 15.303 0.38 −3.84 ±0.69 −2.85 ± 0.60 4.78 ± 0.91 233.4
10 B3 V 259.327,−36.361 14.85 5973935299813148928 0.599 ± 0.046 0.01 ± 0.06 −3.03 ± 0.05 14.240 0.89 −7.12 ±0.75 −5.00 ± 0.60 8.70 ± 0.96 234.9
11 B0 Ib 259.359,−36.247 13.59 5975437198328133888 −0.043 ± 0.090 1.48 ± 0.22 −2.52 ± 0.14 12.307 0.41
12 B1 V 259.359,−36.219 16.23 5975438400927014912 0.614 ± 0.096 0.02 ± 0.13 −1.86 ± 0.09 14.896 0.90 0.78 ± 0.2 0.49 ± 0.15 0.92 ± 0.25 57.8
13 B1 V 259.365,−36.163 15.56 5975438847603624192 0.656 ± 0.082 0.14 ± 0.12 −1.79 ± 0.08 14.310 0.40 2.52 ± 0.56 0.63 ± 0.16 2.59 ± 0.58 75.8
14 B2 V 259.448,−35.896 14.93 5975460803476496384 0.515 ± 0.033 −0.26 ± 0.06 −1.88 ± 0.05 14.388 0.52 −3.55 ±0.38 0.72 ± 0.11 3.62 ± 0.4 281.5
TYC 7370-460-1 O6.5 V 259.564,−34.002 11.80 5978778884750785280 0.552 ± 0.050 −4.86 ± 0.11 −1.36 ± 0.07 10.874 0.14 −22.15±2.67 35.59 ± 4.63 41.92 ± 5.34 328.1
15 B2 V 259.727,−36.018 16.64 5975445135436117760 0.415 ± 0.077 −0.23 ± 0.13 −1.70 ± 0.09 15.414 0.82 −5.91 ±1.68 −0.14 ± 0.05 5.91 ± 1.68 268.7
16 B2 V 259.745,−35.697 15.19 5975488085104930816 0.411 ± 0.039 0.67 ± 0.07 −2.32 ± 0.05 14.672 0.41 −6.05 ±0.89 −12.97 ±1.81 14.31 ± 2.01 205.0
17 B2 V 259.772,−35.703 13.98 5975487844591688704 0.556 ± 0.029 0.25 ± 0.05 −2.02 ± 0.04 13.577 1.01 −0.94 ±0.09 −2.85 ± 0.28 3.00 ± 0.29 198.3
CD-35 11465 B2 IV 259.781,−35.629 11.44 5975494231206615424 −0.716 ± 0.741 −3.03 ± 1.28 −5.88 ± 0.96 11.177 0.10
HD319701 B1 Ib 259.817,−35.902 10.10 5975469560907849728 0.649 ± 0.056 −0.39 ± 0.09 −1.27 ± 0.06 9.500 0.89 3.03 ± 0.51 5.86 ± 2.10 6.60 ± 2.10 27.3
… … … … … … … … … … … … … … …

Notes.

(a)

Star identified with a running number are from Russeil et al. (2017). Stars with an identification are from literature.

(b)

It is the Bayesian distance. The complete table is available at the CDS.

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