Theia 199

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0.08 UTI
0.44
CN
0.3
Cdens
0.75
CC3
0.25
Clit
0.2
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.44 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.2 Likely duplicate

Overview

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Theia 199 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

Liu et al. (2025)
Classified as primordial binary cluster 349 along with UPK_137.

Palma et al. (2025)
Classified as optical pair P572, along with UPK_137.

Cavallo et al. (2024)
Gold 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– 309.434 54.512 1.222 -3.096 -6.732 -20.545
Hunt & Reffert 2024 309.382 54.688 1.206 -3.098 -6.839 -24.486
Cavallo et al. 2024 309.22 53.817 1.211 – – –
Hunt & Reffert 2023 309.382 54.688 1.206 -3.098 -6.839 -24.486

💡 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– 0.83 0.46 1.09 44 0.260 50 – –
Liu et al. 2025 0.83 0.16 – 62 – – – –
Hunt & Reffert 2024 – – – – – 50(1) – –
Cavallo et al. 2024 0.84 0.68 – 44 0.260 – – –
Hunt & Reffert 2023 0.79 0.46 1.09 34 – – – –

(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 444 79.5 309.46 54.4 1.22 -3.11 -6.73 -20.54 0.28

💡 Note: The % column shows the percentage of members that Theia 199 shares with each listed object.

Visualization

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