Table A.3.
Sample of the fourteen GW Vir stars considered in this work. Each column contains information similar to that presented in Table A.2. The spectroscopic effective temperature and surface gravity are those tabulated by Córsico et al. (2019a), unless another reference is indicated. Since PG 2131+066 lacks parallax data from Gaia, we are unable to obtain the Bailer-Jones et al. (2021)’s distance, therefore, we include here the distance derived by Reed et al. (2000) using the spectroscopic parallax of the M star, the primary component of the binary system to which PG 2131+066 belongs.
Name | RA | DEC | V | G | GBP | GRP | S. Type | Teff | log g | π | dBJ | AV | Reference |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(deg) | (deg) | (mag) | (mag) | (mag) | (mag) | (K) | (cgs) | (mas) | (pc) | (mag) | |||
(a) | (b) | (c) | (d) | (e) | (f) | (g) | (h) | (i) | (j) | (k) | (l) | (m) | (n) |
PG 0122+200 | 21.343833 | 20.299097 | 16.845 ± 0.019 | 16.751 | 16.593 | 17.109 | PG 1159 | 80 000 ± 4000 | 7.50 ± 0.50 |
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Werner & Rauch (2014) |
PG 2131+066 | 323.534167 | 6.849331 | 16.577 ± 0.100 | 16.545 | 16.356 | 16.160 | PG 1159 | 95 000 ± 5000 | 7.50 ± 0.50 | ⋯ |
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Werner & Rauch (2014) |
PG 1707+427 | 257.198625 | 42.683578 | 16.757 ± 0.027 | 16.648 | 16.452 | 17.027 | PG 1159 | 85 000 ± 5000 | 7.50 ± 0.50 |
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Werner & Rauch (2014) |
SDSS J075415.12+085232.2 | 118.562991 | 8.875609 | 19.186 ± 0.046 | 18.078 | 18.925 | 19.495 | PG 1159 | 120 000 ± 10 000 | 7.00 ± 0.30 |
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Werner et al. (2014) |
SDSS J034917.41−005919.3 | 57.322537 | −0.988675 | 17.845 ± 0.026 | 17.798 | 17.694 | 17.968 | PG 1159 | 90 000 ± 900 | 7.50 ± 0.01 |
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Hügelmeyer et al. (2006) |
RX J2117.1+3412 | 319.284507 | 34.207616 | 13.120 ± 0.009 | 13.022 | 12.842 | 13.375 | PG 1159 | 170 000 ± 10 000 | 6.00 ± 0.03 |
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Werner et al. (2005) |
HS 2324+3944 | 351.816397 | 40.023175 | 14.821 ± 0.012 | 14.770 | 14.653 | 14.958 | PG41159 | 130 000 ± 10 000 | 6.20 ± 0.20 |
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Dreizler et al. (1996) |
NGC 6905 | 305.595800 | 20.104524 | 14.634 ± 0.026 | 14.597 | 14.443 | 14.637 | [WC3] | 141 000 ± 10 000 | 6.00 ± 0.20 |
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Ciardullo & Bond (1996) |
NGC 2371 | 111.394535 | 29.490675 | 14.853 ± 0.025 | 14.778 | 14.620 | 15.053 | [WO1] | 135 000 ± 10 000 | 6.30 ± 0.20 |
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Herald & Bianchi (2004) |
NGC 1501 | 61.747467 | 60.920631 | 14.329 ± 0.023 | 14.237 | 14.470 | 13.873 | [WO4] | 134 000 ± 10 000 | 6.00 ± 0.20 |
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Koesterke & Hamann (1997) |
TIC 333432673 | 100.315183 | −13.689936 | 15.290 ± 0.021 | 15.215 | 15.058 | 15.492 | PG 1159 | 120 000 ± 10 000 | 7.50 ± 0.50 |
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Uzundag et al. (2021) |
TIC 095332541 | 90.687447 | −13.850989 | 15.413 ± 0.020 | 15.319 | 15.139 | 15.656 | PG 1159 | 120 000 ± 10 000 | 7.50 ± 0.50 |
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Uzundag et al. (2021) |
PG 1159−035 | 180.441555 | −3.7612860 | 15.808 ± 0.015 | 14.693 | 14.485 | 14.080 | PG 1159 | 140 000 ± 5000 | 7.00 ± 0.50 |
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Werner et al. (2011) |
NGC 246 | 11.763925 | −11.871936 | 11.905 ± 0.012 | 11.797 | 11.597 | 12.169 | PG 1159 | 150 000 ± 10 000 | 5.70 ± 0.10 |
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Löbling (2020) |
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