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Table 3.
Basic properties of our PMS CP candidates.
| Gaia DR3 | RA ICRS | Dec ICRS | ϖ | Cluster | SpT our | SpT literature |
|---|---|---|---|---|---|---|
| 121406905707934464 | 52.3324400 | 31.4158037 | 3.4802 ± 0.0237 | NGC 1333 | B9 III-V Si | B8-9 Si He-wk (1) |
| 216648703146774016 | 56.4495623 | 32.0162390 | 3.0693 ± 0.0325 | IC 348 | A0 SiSr (2) | |
| 3019972890876467968 | 92.0529125 | −6.1956720 | 1.2045 ± 0.0172 | OC 357 | B8 IV-V Si: | B6 IV Si (3) |
| 3368982075084757632 | 94.8562983 | 15.3365834 | 0.2395 ± 0.0409 | UBC 438 | B9 Ve SrSiEu | A2 V (4) |
| 3326717260430731648 | 100.2148105 | 9.8637002 | 1.3310 ± 0.0365 | NGC 2264 | B6 He var (2) | |
| 6244725050721030528 | 245.0228316 | −20.0565075 | 7.6496 ± 0.0297 | HSC 2931 | B9 SiCrSr (2) | |
| 5966515967154648064 | 253.4669125 | −41.8150331 | 0.5817 ± 0.0205 | NGC 6231 | A (2) | |
| 2244529022468154880 | 305.7257939 | 64.1840742 | 2.1286 ± 0.0137 | UPK 160 | A0 Si (2) |
References. (1) Potravnov et al. (2023b), (2) Renson & Manfroid (2009), (3) Shang et al. (2022), (4) Zhang et al. (2022).
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