Table 4.
Galactocentric distances derived from Gaia DR2 parallaxes (Gaia Collaboration 2018), Gaia DR2 parallaxes combined with a geometrical prior (Bailer-Jones et al. 2018), or period-Wesenheit relations in the near-infrared (Inno et al. 2013; Genovali et al. 2014).
| Star | Rg kpc Gaia parallax | Rg kpc Gaia parallax with prior | Rg kpc PW (NIR) | |
|---|---|---|---|---|
| V371 | Per | 12.454 | 11.315 | |
| TU | Cas | 8.510 | 8.492 | 8.398 |
| V825 | Cas | 12.084 | 11.135 | |
| AS | Cas | 9.883 | 9.969 | 9.662 |
| Gaia | 1 | 10.757 | 9.502 | |
| DZ | CMa | 11.575 | 11.026 | |
| OGLE-BLG-CEP-21 | 3.652 | 3.622 | ||
| OGLE-BLG-CEP-03 | 0.611 | 2.878 | ||
| V458 | Sct | 6.075 | 6.165 | 6.488 |
| V367 | Sct | 5.795 | 5.913 | 6.332 |
| EW | Sct | 7.503 | 7.508 | 7.580 |
| BQ | Ser | 6.952 | 6.982 | 7.169 |
| OGLE-GD-CEP-0009 | 9.559 | |||
| EY | Car | 7.573 | 7.559 | 7.563 |
| GZ | Car | 7.728 | 7.707 | 7.681 |
| V701 | Car | 7.777 | 7.769 | 7.769 |
| BK | Cen | 7.156 | 7.176 | 7.268 |
| UZ | Cen | 7.406 | 7.423 | 7.465 |
| OGLE-GD-CEP-0012 | 10.333 | 8.422 | ||
| Y | Car | 7.734 | 7.694 | 7.682 |
| Gaia | 2 | 7.571 | 7.581 | |
| AX | Vel | 8.285 | 8.264 | 8.120 |
| AP | Vel | 8.352 | 8.324 | 8.291 |
| BE | Pup | 12.411 | 11.512 | |
| VX | Pup | 8.900 | 8.857 | 8.703 |
| U | TrA | 7.068 | 7.093 | 7.207 |
| Gaia | 3 | 6.832 | 6.482 | |
| OGLE-GD-CEP-0016 | 8.563 | |||
| V1210 | Cen | 6.504 | 6.576 | 6.775 |
| V901 | Mon | 8.142 | 8.141 | |
Notes. Distances have been computed assuming a Galactocentric distance of 7.94 kpc for the Sun.
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