Theia 1746

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0.01 UTI
0.26
CN
0.22
Cdens
0.62
CC3
0.0
Clit
0.04
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.04 Very likely duplicate

Overview

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Theia 1746 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P46, along with HSC_2858.

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– 257.835 -41.745 0.367 -0.529 -1.534 -21.262
Hunt & Reffert 2024 257.707 -41.854 0.365 -0.497 -1.467 -50.015
Cavallo et al. 2024 257.779 -41.798 0.364 – – –
Hunt & Reffert 2023 257.707 -41.854 0.365 -0.497 -1.467 -50.015

💡 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– 2.355 3.41 1.76 121 0.540 707 – –
Hunt & Reffert 2024 – – – – – 707(1) – –
Cavallo et al. 2024 2.24 3.43 – 166 0.540 – – –
Hunt & Reffert 2023 2.47 3.39 1.76 76 – – – –

(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 2507 96.2 257.81 -41.77 0.37 -0.57 -1.54 -24.79 0.26

💡 Note: The % column shows the percentage of members that Theia 1746 shares with each listed object.

Visualization

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