Theia 267

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0.24 UTI
0.54
CN
0.28
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.54 Moderately populated
  • Cdens 0.28 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 267 is a moderately populated, loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Palma et al. (2025)
Part of multiple system G241, along with HSC_1743 and Theia_361.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 105.897 -7.948 1.412 -3.301 2.48 43.595
Hunt & Reffert 2024 105.867 -8.017 1.424 -3.301 2.479 44.314
Hunt & Reffert 2023 105.867 -8.017 1.424 -3.301 2.479 44.314

💡 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– 0.66 0.17 0.52 223 – 46 – –
Hunt & Reffert 2024 – – – – – 46(1) – –
Hunt & Reffert 2023 0.66 0.17 0.52 223 – – – –

(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 3723 41.4 105.92 -7.46 1.41 -3.38 2.42 44.83 0.0

💡 Note: The % column shows the percentage of members that Theia 267 shares with each listed object.

Visualization

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