Theia 12

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0.20 UTI
0.67
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.42
Cdup
Stellar density (N50/rad) 8.0 [N/pc2]
  • CN 0.67 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.42 Possibly duplicate

Overview

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Theia 12 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P168, along with UPK_38.

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 281.947 -2.396 1.584 0.222 -6.238 6.148
Hunt & Reffert 2024 282.102 -2.382 1.569 0.139 -6.178 6.12
Cavallo et al. 2024 281.825 -2.246 1.571 – – –
Hunt & Reffert 2023 282.102 -2.382 1.569 0.139 -6.178 6.12

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 0.65 3.52 2.91 6 0.080 262 – –
Hunt & Reffert 2024 – – – – – 262(1) – –
Cavallo et al. 2024 0.69 3.85 – 7 0.080 – – –
Hunt & Reffert 2023 0.61 3.19 2.91 5 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1245 58.3 282.06 -2.44 1.59 0.31 -6.31 5.34 0.41
Ryu 269 10.7 282.18 -2.46 1.6 0.31 -6.01 43.62 0.3

💡 Note: The % column shows the percentage of members that Theia 12 shares with each listed object.

Visualization

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