Table 1.
Derived data for the sample stars.
| Name | Gaia EDR3 source id | AV | AV | AV | Jo | Kso | Distance | Mbol | Z | RGC | Vr | Vθ | Vz | Pop |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (mag) | (mag) | (mag) | (mag) | (mag) | (pc) | (mag) | (kpc) | (kpc) | (km s−1) | (km s−1) | (km s−1) | |||
| N-type | ||||||||||||||
| R Scl | 5016138145186249088 | 0.04 | 0.08 | ... | 1.43 | −0.12 | 387.02 | −4.89 | −0.36 | 8.20 | −60.79 | 214.43 | 15.14 | 0 |
| AQ Sgr | 4180404407794509056 | 0.47 | 0.26 | 0.45 | 2.43 | 0.71 | 556.30 | −4.88 | −0.13 | 7.85 | −8.70 | 261.10 | −1.70 | 0 |
| TX Psc | 2743004129429424000 | 0.09 | 0.11 | 0.07 | 0.79 | −0.52 | 244.28 | −4.62 | −0.18 | 8.19 | −52.71 | 251.02 | −7.51 | 0 |
| R Lep | 2987082722815713792 | 0.12 | 0.25 | 0.35 | 2.11 | 0.12 | 446.33 | −4.96 | −0.21 | 8.50 | −4.52 | 230.31 | 8.82 | 0 |
| RT Cap | 6853966780133956096 | 0.43 | 0.28 | 0.45 | 2.25 | 0.25 | 540.51 | −4.92 | −0.23 | 7.74 | 19.86 | 212.20 | −1.21 | 0 |
| RV Cyg | 1952830855365548416 | 0.46 | 0.49 | 0.68 | 1.68 | 0.69 | 670.01 | −6.09 | −0.11 | 8.17 | −19.86 | 251.43 | 7.40 | 0 |
| S Sct | 4251993571231284224 | 0.59 | 0.26 | 0.24 | 1.86 | 0.56 | 415.84 | −4.87 | 0.00 | 7.81 | −5.39 | 245.99 | −9.20 | 0 |
| SS Vir | 3699854707618766848 | 0.07 | 0.07 | 0.01 | 2.32 | 0.82 | 547.87 | −5.06 | 0.51 | 8.10 | −15.41 | 247.04 | 9.44 | 0 |
| ST Cam | 483958671558728576 | 0.47 | 0.25 | 0.65 | 2.01 | 0.42 | 586.36 | −5.42 | 0.17 | 8.63 | −7.87 | 243.52 | −7.31 | 0 |
| TU Gem | 3427006189904854656 | 0.78 | 0.66 | 1.13 | 2.20 | 0.73 | 1101.36 | −6.44 | 0.09 | 9.27 | 32.12 | 210.41 | −5.98 | 0 |
| ... |
Notes. Pop: membership probability higher than 80% for thin disc (0), thick disc (1), halo (2), ambiguous or no Gaia DR2 Vrad available (blank, see text). Columns 3–5 show the extinction values from Lallement et al. (2019), Drimmel et al. (2003), and Green et al. (2019) Galactic models, respectively. The Jo and Kso magnitudes are those corrected for extinction according to Lallement et al. (2019). The complete version of this table is only available at the CDS.
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