Theia 3329

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0.12 UTI
0.26
CN
0.68
Cdens
0.75
CC3
0.0
Clit
0.35
Cdup
Radius (P>50% members) 9.7 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.68 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.35 Possibly duplicate

Overview

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Theia 3329 is a poorly populated, moderately dense object of high 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 (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.

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 – 255.374 -25.692 1.022 -0.599 0.304 -18.548
Hunt & Reffert 2024 255.407 -25.706 1.011 -0.728 0.332 -16.086
Cavallo et al. 2024 255.341 -25.678 1.017 – – –
Hunt & Reffert 2023 255.407 -25.706 1.011 -0.728 0.332 -16.086

💡 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 – – – – – 77* – –
Cavallo et al. 2024 0.99 0.84 – 115 0.210 – – –
Hunt & Reffert 2023 0.95 0.51 0.58 291 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 291 65.4 255.37 -25.72 1.02 -0.54 0.34 -15.25 0.23

💡 Note: The % column shows the percentage of members that Theia 3329 shares with each listed object.

Visualization

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