Theia 5320

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0.10 UTI
0.25
CN
0.61
Cdens
0.38
CC3
0.0
Clit
0.4
Cdup
Stellar density (N50/rad) 3.0 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.61 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.4 Possibly duplicate

Overview

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Theia 5320 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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– 126.649 -33.711 0.742 -4.848 4.406 37.338
Hunt & Reffert 2024 126.596 -33.743 0.732 -4.833 4.345 46.128
Cavallo et al. 2024 126.526 -33.493 0.737 – – –
Hunt & Reffert 2023 126.596 -33.743 0.732 -4.833 4.345 46.128

💡 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– 1.355 0.41 0.95 32 -0.180 95 – –
Hunt & Reffert 2024 – – – – – 95(1) – –
Cavallo et al. 2024 1.41 0.46 – 23 -0.180 – – –
Hunt & Reffert 2023 1.30 0.36 0.95 42 – – – –

(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 223 60.0 126.59 -33.66 0.73 -4.87 4.43 35.06 0.11

💡 Note: The % column shows the percentage of members that Theia 5320 shares with each listed object.

Visualization

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