Theia 323

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0.18 UTI
0.25
CN
0.09
Cdens
0.5
CC3
0.03
Clit
1.0
Cdup
Core radius and density 2.3 [pc], 0.5 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 323 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, above 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.

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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (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– 194.176 -55.692 2.049 -13.69 -3.296 3.254
Cavallo et al. 2024 191.29 -55.715 2.017 – – –
Hunt & Reffert 2023 194.203 -55.763 2.011 -13.905 -3.07 -0.661
Kounkel & Covey 2019 195.033 -57.111 1.909 – – -5.275

💡 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– 0.48 0.5 0.98 100 0.030 – – –
Cavallo et al. 2024 0.48 0.69 – 95 0.030 – – –
Hunt & Reffert 2023 0.47 0.22 0.98 128 – – – –
Kounkel & Covey 2019 0.52 0.50 – 100 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 450 48.0 194.43 -55.77 2.06 -13.54 -3.65 0.01 0.15

💡 Note: The % column shows the percentage of members that Theia 323 shares with each listed object.

Visualization

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