Theia 1873

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0.19 UTI
0.0
CN
0.19
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 13.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 1873 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported 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.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 206.598 -62.491 0.805 -3.69 -2.58 -7.04
Cavallo et al. 2024 206.68 -62.522 0.8 – – –
Hunt & Reffert 2023 206.582 -62.688 0.802 -3.697 -2.568 -4.111

💡 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] Bfr BSS
Cavallo et al. 2024 1.20 0.19 – 191 0.230 – – –
Hunt & Reffert 2023 1.21 0.42 0.73 172 – – – –

Visualization

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