Theia 667

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0.42 UTI
0.42
CN
0.45
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 18.7 [arcmin]
  • CN 0.42 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 667 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Close Moderate 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 – 352.604 64.014 1.262 -4.882 -4.875 -9.579
Hunt & Reffert 2024 352.486 63.993 1.249 -4.883 -4.763 -8.051
Cavallo et al. 2024 352.691 64.181 1.257 – – –
Hunt & Reffert 2023 352.486 63.993 1.249 -4.883 -4.763 -8.051
He et al. 2022 352.334 64.068 1.263 -4.888 -4.823 –

💡 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 – – – – – 144* – –
Cavallo et al. 2024 0.82 1.17 – 191 0.300 – – –
Hunt & Reffert 2023 0.75 0.95 1.53 124 – – – –
He et al. 2022 – 1.25 – 112 – – – –

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

Visualization

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