Theia 3263

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0.02 UTI
0.27
CN
0.55
Cdens
0.5
CC3
0.0
Clit
0.07
Cdup
Radius (P>50% members) 10.5 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.55 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.07 Very likely duplicate

Overview

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Theia 3263 is a poorly populated, moderately dense object of intermediate 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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 – 220.55 -58.393 0.974 -2.091 -1.758 -6.431
Hunt & Reffert 2024 220.545 -58.379 0.959 -2.15 -1.812 -3.144
Cavallo et al. 2024 220.168 -58.469 0.968 – – –
Hunt & Reffert 2023 220.545 -58.379 0.959 -2.15 -1.812 -3.144

💡 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 – – – – – 84* – –
Cavallo et al. 2024 0.99 1.25 – 339 0.190 – – –
Hunt & Reffert 2023 0.98 0.94 0.85 268 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 357 92.6 220.5 -58.43 0.98 -2.08 -1.77 -1.2 0.33

💡 Note: The % column shows the percentage of members that Theia 3263 shares with each listed object.

Visualization

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