Theia 1082

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0.11 UTI
0.0
CN
0.28
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 16.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.28 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 1082 is a sparse, loose object of low C3 quality. Its parallax locates it at a close distance, above 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.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 193.248 -59.062 1.194 -9.867 -3.502 -22.305
Hunt & Reffert 2024 193.652 -58.96 1.179 -9.883 -3.399 -20.713
Cavallo et al. 2024 192.84 -58.986 1.179 – – –
Hunt & Reffert 2023 193.652 -58.96 1.179 -9.883 -3.399 -20.713

💡 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
Hunt & Reffert 2024 – – – – – 90* – –
Cavallo et al. 2024 0.82 0.72 – 107 0.170 – – –
Hunt & Reffert 2023 0.80 0.36 0.52 158 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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