Theia 4208

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0.60 UTI
0.65
CN
0.83
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.6 [arcmin]
  • CN 0.65 Moderately populated
  • Cdens 0.83 Dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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Theia 4208 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively 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 – 280.441 -19.653 0.636 1.608 1.003 -24.345
Hu & Soubiran 2025 280.441 -19.644 – – – –
Hunt & Reffert 2024 280.417 -19.647 0.629 1.611 0.979 -22.182
Cavallo et al. 2024 280.441 -19.644 0.63 – – –
Hunt & Reffert 2023 280.417 -19.647 0.629 1.611 0.979 -22.182

💡 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 – – – – -0.220* – – –
Hunt & Reffert 2024 – – – – – 256* – –
Cavallo et al. 2024 1.39 1.18 – 741 0.000 – – –
Hunt & Reffert 2023 1.52 0.91 0.53 619 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3251 71.2 280.44 -19.68 0.64 1.62 1.0 -24.94 0.0

💡 Note: The % column shows the percentage of members that Theia 4208 shares with each listed object.

Visualization

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