Theia 624

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0.07 UTI
0.0
CN
0.06
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Core radius and density 2.4 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.25 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 624 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, near 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: 0.97 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (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– 247.692 -44.519 1.514 -1.643 -7.565 -18.792
Cavallo et al. 2024 247.955 -44.658 1.523 – – –
Hunt & Reffert 2023 247.45 -44.55 1.526 -1.543 -7.547 -29.8
Kounkel & Covey 2019 248.905 -45.301 2.19 – – -4.447

💡 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– 0.62 0.58 0.32 120 0.150 – – –
Cavallo et al. 2024 0.66 0.84 – 120 0.150 – – –
Hunt & Reffert 2023 0.62 0.58 0.32 105 – – – –
Kounkel & Covey 2019 0.45 0.58 – 303 – – – –

Visualization

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