Theia 771

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0.45 UTI
0.55
CN
0.57
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 18.3 [arcmin]
  • CN 0.55 Moderately populated
  • Cdens 0.57 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 771 is a moderately populated, moderately dense object of intermediate 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, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
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 – 199.083 -59.231 1.163 -14.952 -1.81 -11.525
Hu & Soubiran 2025 199.533 -59.201 – – – –
Hunt & Reffert 2024 198.889 -59.23 1.164 -14.932 -1.808 -12.502
Cavallo et al. 2024 199.533 -59.201 1.161 – – –
Hunt & Reffert 2023 198.889 -59.23 1.164 -14.932 -1.808 -12.502

💡 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
Hu & Soubiran 2025 – – – – -0.140* – – –
Hunt & Reffert 2024 – – – – – 50* – –
Cavallo et al. 2024 0.78 0.47 – 525 0.640 – – –
Hunt & Reffert 2023 0.82 0.66 0.56 326 – – – –

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

Visualization

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