Theia 713

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0.08 UTI
0.0
CN
0.09
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Core radius and density 1.2 [pc], 0.4 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.25 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 713 is a sparse, very loose object of low 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.

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.

Palma et al. (2025)
Classified as optical pair P587, along with UPK_233.

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– 7.442 68.42 2.105 -6.213 -4.718 -21.724
Cavallo et al. 2024 5.983 68.376 2.112 – – –
Hunt & Reffert 2023 7.541 68.412 2.112 -6.118 -4.741 -20.415
Kounkel & Covey 2019 10.109 67.056 2.203 – – -11.723

💡 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– 0.45 0.89 1.78 327 -0.060 – – –
Cavallo et al. 2024 0.47 1.20 – 309 -0.060 – – –
Hunt & Reffert 2023 0.45 0.89 1.78 327 – – – –
Kounkel & Covey 2019 0.45 0.60 – 355 – – – –

Visualization

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