Theia 1203

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0.12 UTI
0.25
CN
0.05
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Core radius and density 2.4 [pc], 0.2 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.05 Very loose
  • CC3 0.25 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 1203 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.73 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.73 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 281.101 -57.38 2.416 5.645 -24.918 -21.367
Cavallo et al. 2024 282.278 -56.888 2.454 – – –
Hunt & Reffert 2023 281.015 -57.178 2.443 5.64 -24.905 -22.844
Kounkel & Covey 2019 282.156 -57.339 2.459 – – -16.685

💡 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– 0.41 0.24 0.73 279 0.360 – – –
Cavallo et al. 2024 0.42 0.41 – 200 0.360 – – –
Hunt & Reffert 2023 0.39 0.19 0.73 279 – – – –
Kounkel & Covey 2019 0.41 0.24 – 1200 – – – –

Visualization

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