Table D.1
Results of the spectroscopic analysis of the stars in the sample (extract).
ID | 1 | b | SpCa | υ sin ib | υcmac | Teff | log𝑔d | 1 | ξ | 1 | YHe | 1 | log Q | q | Ref. file | SNR |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
[deg] | [deg] | [km s−1] | [km s−1] | [K] | [km s−1] | |||||||||||
HD 164032 | 0.8767 | −3.237 | Bl/2Ib | 108 | 50 | ![]() |
![]() |
= | 18 | = | ![]() |
< | ![]() |
2 | HD164032_20220830_201330_M_V85000_log | 106 |
HD 164019 | 1.9099 | −2.6166 | 09.5IVp | 78 | 46 | ![]() |
![]() |
= | 15 | = | ![]() |
= | ![]() |
1 | HD164019_20080608_075144_F_V48000 | 183 |
HD 163613 | 2.0881 | −1.9638 | Β H/II | 71 | 78 | ![]() |
![]() |
= | 20 | = | ![]() |
= | ![]() |
1 | HD163613_20200804_213522_N_V25000 | 96 |
HD 160430 | 3.7823 | 3.5878 | Β 2II | 20 | 46 | ![]() |
![]() |
= | 13 | = | ![]() |
< | ![]() |
3 | HD160430_20200802_220513_N_V25000 | 96 |
HD 164741 | 5.164 | −1.6449 | B1III(2) | 20 | 32 | ![]() |
![]() |
= | 8 | = | ![]() |
< | ![]() |
1 | HD164741_20180731_223907_M_V85000 | 38 |
HD 173502 | 5.3641 | −12.2722 | B0.5III(2) | 131 | 22 | ![]() |
![]() |
= | 13 | = | ![]() |
< | ![]() |
3 | HD173502_20190710_003102_N_V25000 | 93 |
HD 156779 | 5.4256 | 10.3249 | Β 211 | 97 | 39 | ![]() |
![]() |
= | 13 | = | ![]() |
< | ![]() |
1 | HD156779_20210621_224538_M_V85000_log | 80 |
HD 168941 | 5.821 | −6.3128 | 09.5IVp | 107 | 91 | ![]() |
![]() |
= | 16 | = | ![]() |
< | ![]() |
1 | HD168941_20060512_083253_F_V48000 | 363 |
HD 165016 | 5.8521 | −1.5791 | B0V(2) | 19 | 21 | ![]() |
![]() |
= | 6 | = | ![]() |
> | ![]() |
1 | HD165016_20200803_211628_N_V25000 | 109 |
HD 168750 | 6.1891 | −5.8526 | Β IIb | 33 | 50 | ![]() |
![]() |
= | 13 | = | ![]() |
< | ![]() |
1 | HD168750_20220826_215128_M_V85000_log | 84 |
HD 149757 | 6.2812 | 23.5877 | 09.2IVnn | 410 | 0 | ![]() |
![]() |
= | 16 | = | ![]() |
= | ![]() |
1 | HD149757_20210622_234421_M_V85000_log | 435 |
HD 164018 | 6.6528 | 0.1591 | Bl/2Ib | 142 | 38 | ![]() |
![]() |
= | 15 | = | ![]() |
< | ![]() |
1 | HD164018_20180920_215654_N_V25000 | 70 |
HD 165132 | 6.7522 | −1.2103 | 09.7V(2) | 127 | 20 | ![]() |
![]() |
= | 12 | = | ![]() |
< | ![]() |
1 | HD165132_20190709_222717_N_V67000 | 73 |
HD 164971 | 6.8868 | −0.9279 | BOIa | 43 | 76 | ![]() |
![]() |
= | 16 | = | ![]() |
< | ![]() |
1 | HD164971_20110902_222249_M_V85000 | 60 |
HD 163892 | 7.1516 | 0.6161 | 09.5IV(n) | 216 | 0 | ![]() |
![]() |
= | 12 | = | ![]() |
< | ![]() |
1 | HD163892_20210623_001114_M_V85000_log | 142 |
HD 164402 | 7.1621 | −0.0339 | B01b(3) | 54 | 86 | ![]() |
![]() |
= | 18 | = | ![]() |
= | ![]() |
1 | HD164402_20220829_203450_M_V85000_log | 144 |
HD 164637 | 7.3435 | −0.2284 | B0Ib/II | 35 | 72 | ![]() |
![]() |
= | 15 | = | ![]() |
< | ![]() |
1 | HD164637_20130821_042119_F_V48000 | 327 |
HD 164359 | 7.6967 | 0.338 | BUI | 77 | 35 | ![]() |
![]() |
= | 9 | = | ![]() |
< | ![]() |
2 | HD164359_20220830_210910_M_V85000_log | 131 |
HD 158661 | 8.2908 | 9.0476 | Β0ΙΙ | 60 | 96 | ![]() |
![]() |
= | 22 | = | ![]() |
= | ![]() |
1 | HD158661_20210623_010823_M_V85000_log | 151 |
HD 165812 | 8.476 | −1.1091 | B1/2II | 42 | 34 | ![]() |
![]() |
= | 8 | = | ![]() |
< | ![]() |
1 | HD165812_20200803_215831_N_V25000 | 113 |
HD 166852 | 8.5074 | −2.3235 | B01a/ab | 45 | 130 | ![]() |
![]() |
= | 16 | = | ![]() |
< | ![]() |
1 | HD166852_20190709_220222_N_V67000 | 46 |
HD 159864 | 8.5231 | 7.3825 | Β IIb | 88 | 98 | ![]() |
![]() |
= | 18 | = | ![]() |
< | ![]() |
1 | HD159864_20200502_050638_N_V25000 | 110 |
HD 165516 | 8.9268 | −0.4446 | Bl/2Ib | 47 | 67 | ![]() |
![]() |
= | 17 | = | ![]() |
= | ![]() |
1 | HD165516_20200803_212544_N_V46000 | 144 |
HD 165892 | 9.1729 | −0.8113 | Β 211 | 74 | 42 | ![]() |
![]() |
= | 11 | = | ![]() |
< | ![]() |
1 | HD165892_20130412_050607_M_V85000 | 62 |
HD 149363 | 9.8524 | 26.6906 | Bl/2Ib | 88 | 62 | ![]() |
![]() |
= | 16 | = | ![]() |
< | ![]() |
1 | HD149363_20190707_211718_N_V25000 | 194 |
HD 164438 | 10.3529 | 1.7886 | 09.2IV | 61 | 105 | ![]() |
![]() |
= | 13 | = | ![]() |
< | ![]() |
1 | HD164438_20080514_092403_F_V48000 | 303 |
HD 166546 | 10.358 | -0.9242 | 09.5IV | 31 | 73 | ![]() |
![]() |
= | 12 | = | ![]() |
< | ![]() |
1 | HD166546_20080609_082259_F_V48000 | 284 |
HD 167264 | 10.4557 | −1.7408 | 09.7Iab | 80 | 67 | ![]() |
![]() |
= | 22 | = | ![]() |
= | ![]() |
1 | HD167264_20100907_202837_N_V46000 | 273 |
Notes. (a)We adopted the recommended spectral classification quoted in the SIMBAD astronomical database (Wenger et al. 2000) except for the cases indicated with an upper index and the following: (1) de Burgos et al. (2020); (2) de Burgos et al. (2023); (3) Negueruela et al. (2024). For HD 168021, HD 168183, and HD187879, the SIMBAD classification included a second component, but we have only included the first. In the case of the O-type stars, most of the classifications are adopted from the GOSSS series of papers (Sota et al. 2011, 2014; Maíz Apellániz et al. 2016). (b)We adopt a global uncertainty for υ sin ì of 15 km s−1 based on the average value. (c)We adopt a global uncertainty for υmíc of 20 km s−1 based on the average value. Based on the results by Simón-Díaz & Herrero (2014), we assigned = 0 km s−1 to those cases in which υ sin i > 180 km s−1. (d)The values of log 𝑔 have not been corrected for centrifugal acceleration. The full table is available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/.
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