Theia 3669

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0.02 UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.03
Cdup
Stellar density (N50/rad) 17.1 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.03 Very likely duplicate

Overview

â„šī¸
Theia 3669 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, metal-poor, 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.

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– 243.504 -52.959 0.308 -2.083 -1.87 -25.516
Hunt & Reffert 2024 243.497 -52.965 0.311 -2.089 -1.862 -18.016
Cavallo et al. 2024 243.512 -52.959 0.312 – – –
Hunt & Reffert 2023 243.497 -52.965 0.311 -2.089 -1.862 -18.016

💡 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– 2.555 2.325 2.54 190 -0.670 1662 – –
Hunt & Reffert 2024 – – – – – 1662(1) – –
Cavallo et al. 2024 2.17 2.57 – 234 -0.670 – – –
Hunt & Reffert 2023 2.94 2.08 2.54 147 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1543 96.8 243.51 -52.96 0.31 -2.08 -1.87 -26.02 0.16
UFMG 11 74.5 243.51 -52.96 0.3 -2.08 -1.9 -25.52 0.55

💡 Note: The % column shows the percentage of members that Theia 3669 shares with each listed object.

Visualization

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