Theia 4165

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0.07 UTI
0.28
CN
0.6
Cdens
0.5
CC3
0.0
Clit
0.25
Cdup
Stellar density (N50/rad) 3.0 [N/pc2]
  • CN 0.28 Poorly populated
  • Cdens 0.6 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.25 Possibly duplicate

Overview

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Theia 4165 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below 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.

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 99999– 328.584 46.954 0.668 1.228 -2.33 -11.421
Hunt & Reffert 2024 328.586 46.965 0.67 1.245 -2.368 -11.527
Cavallo et al. 2024 328.123 46.817 0.67 – – –
Hunt & Reffert 2023 328.586 46.965 0.67 1.245 -2.368 -11.527

💡 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] Bfrac BSS
UCC 99999– 1.48 0.63 0.77 473 0.340 103 – –
Hunt & Reffert 2024 – – – – – 103(1) – –
Cavallo et al. 2024 1.53 0.81 – 339 0.340 – – –
Hunt & Reffert 2023 1.43 0.45 0.77 607 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 1 75.0 328.51 46.91 0.67 1.26 -2.34 -13.97 0.2

💡 Note: The % column shows the percentage of members that Theia 4165 shares with each listed object.

Visualization

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