Theia 589

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0.13 UTI
0.0
CN
0.04
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 4.9 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 589 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate 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)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 268.614 -22.192 1.077 2.983 -0.666 -16.088
Hunt & Reffert 2024 268.657 -22.007 1.069 2.972 -0.653 -50.763
Cavallo et al. 2024 268.623 -22.284 1.07 – – –
Hunt & Reffert 2023 268.657 -22.007 1.069 2.972 -0.653 -50.763
Kounkel & Covey 2019 268.713 -22.309 1.188 – – 3.424

💡 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– 0.86 1.45 0.56 140 -0.100 60 – –
Hunt & Reffert 2024 0.86 1.45 0.56 62 – 60(1) – –
Cavallo et al. 2024 1.06 1.21 – 219 -0.100 – – –
Hunt & Reffert 2023 0.86 1.45 0.56 62 – – – –
Kounkel & Covey 2019 0.84 1.72 – 226 – – – –

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

Visualization

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