Theia 2966

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0.19 UTI
0.0
CN
0.44
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.44 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 2966 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It was recently reported in the literature.

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.

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– 110.158 -14.016 0.596 -0.753 0.645 10.704
Hunt & Reffert 2024 110.159 -14.031 0.59 -0.73 0.643 10.706
Cavallo et al. 2024 110.116 -14.034 0.602 – – –
Hunt & Reffert 2023 110.159 -14.031 0.59 -0.73 0.643 10.706

💡 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– 1.745 0.295 0.56 230 0.690 74 – –
Hunt & Reffert 2024 – – – – – 74(1) – –
Cavallo et al. 2024 1.87 0.00 – 355 0.690 – – –
Hunt & Reffert 2023 1.62 0.59 0.56 105 – – – –

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

Visualization

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