Theia 4367

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0.05 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.12
Cdup
Stellar density (N50/rad) 8.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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Theia 4367 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

(*): The parallax distance estimate (~4.63 kpc) differs significantly from the median photometric distance (~3.32 kpc).

Cavallo et al. (2024)
Silver 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– 176.636 -62.061 0.216 -6.678 1.094 -0.844
Hunt & Reffert 2024 176.631 -62.045 0.224 -6.668 1.106 -15.611
Cavallo et al. 2024 176.628 -62.056 0.227 – – –
Hunt & Reffert 2023 176.631 -62.045 0.224 -6.668 1.106 -15.611

💡 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– 3.32 1.995 1.8 324 -0.560 551 – –
Hunt & Reffert 2024 – – – – – 551(1) – –
Cavallo et al. 2024 2.70 2.10 – 447 -0.560 – – –
Hunt & Reffert 2023 3.94 1.89 1.80 202 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1608 88.0 176.63 -62.06 0.22 -6.68 1.09 -10.18 0.35

💡 Note: The % column shows the percentage of members that Theia 4367 shares with each listed object.

Visualization

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