Theia 2087

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0.18 UTI
0.26
CN
0.26
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 14.9 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.26 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 2087 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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 Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 133.846 -42.258 0.964 -7.495 5.658 19.247
Hunt & Reffert 2024 133.626 -42.126 0.961 -7.516 5.668 24.496
Cavallo et al. 2024 133.774 -42.214 0.959 – – –
Hunt & Reffert 2023 133.626 -42.126 0.961 -7.516 5.668 24.496

💡 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 – – – – – 119* – –
Cavallo et al. 2024 1.21 1.81 – 47 0.340 – – –
Hunt & Reffert 2023 1.00 1.67 2.23 148 – – – –

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

Visualization

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