Table 5
Distances and luminosities of the Galactic sample, derived using the PLC relationship.
| Star | Ppuls. | E(B−V) | Teff | Distance | Luminosity |
| (d) | (mag) | (K) | (kpc) | (L⊙) | |
|
|
|||||
| DY Ori | 30.4 | 0.9 ± 0.1 | 5500 | 2.1 ± 0.21 | 1350 ± 250 |
| EP Lyr | 41.6 | 0.4 ± 0.2 | 6200 | 3.0 ± 0.30 | 1700 ± 300 |
| HP Lyr | 68.4 | 0.1 ± 0.1 | 5900 | 6.7 ± 0.38 | 3900 ± 400 |
| IRAS 17038 | 37.9 | 0.3 ± 0.1 | 5000 | 3.8 ± 0.46 | 3000 ± 700 |
| IRAS 09144 | 50.3 | 1.4 ± 0.2 | 5500 | 2.5 ± 0.36 | 2800 ± 800 |
| TW Cam | 43.1 | 0.3 ± 0.1 | 4700 | 2.7 ± 0.26 | 3000 ± 600 |
Notes. Column 2 shows the fundamental pulsation period (P0). Column 3 is the amount of extinction towards each object obtained from the reddened SED model. The temperatures used for the SED fitting are shown in Col. 4. The distances and luminosities are shown in the last 2 columns, respectively.
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