Theia 436

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0.08 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.03
Clit
1.0
Cdup
Core radius and density 2.0 [pc], 0.4 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.03 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 436 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very 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: 0.99 (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– 219.432 -65.803 4.643 -14.93 -18.897 11.543
Cavallo et al. 2024 220.215 -65.56 4.645 – – –
Hunt & Reffert 2023 221.869 -65.401 4.657 -15.31 -18.915 13.767
Kounkel & Covey 2019 218.494 -65.55 4.143 – – -14.869

💡 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– 0.22 0.36 0.34 120 0.180 – – –
Cavallo et al. 2024 0.21 0.37 – 120 0.180 – – –
Hunt & Reffert 2023 0.22 0.09 0.34 108 – – – –
Kounkel & Covey 2019 0.24 0.36 – 172 – – – –

Visualization

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