Theia 2062

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0.19 UTI
0.54
CN
0.88
Cdens
0.75
CC3
0.0
Clit
0.43
Cdup
Radius (P>50% members) 10.3 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 0.88 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.43 Possibly duplicate

Overview

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Theia 2062 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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 – 243.476 -51.276 0.824 0.157 -2.193 -11.466
Hunt & Reffert 2024 243.51 -51.184 0.822 0.146 -2.174 -19.313
Cavallo et al. 2024 243.429 -51.269 0.826 – – –
Hunt & Reffert 2023 243.51 -51.184 0.822 0.146 -2.174 -19.313

💡 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 – – – – – 246* – –
Cavallo et al. 2024 1.03 1.36 – 100 -0.180 – – –
Hunt & Reffert 2023 1.14 0.96 0.47 88 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1065 56.9 243.44 -51.25 0.82 0.16 -2.17 -12.49 0.35

💡 Note: The % column shows the percentage of members that Theia 2062 shares with each listed object.

Visualization

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