Theia 4371

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0.03 UTI
0.0
CN
0.19
Cdens
0.5
CC3
0.0
Clit
0.2
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.2 Likely duplicate

Overview

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Theia 4371 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate 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 – 147.12 -51.294 0.292 -5.064 3.593 –
Hunt & Reffert 2024 147.184 -51.261 0.283 -5.074 3.613 –
Cavallo et al. 2024 147.117 -51.302 0.286 – – –
Hunt & Reffert 2023 147.184 -51.261 0.283 -5.074 3.613 –

💡 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 – – – – – 189* – –
Cavallo et al. 2024 2.94 1.78 – 224 -0.110 – – –
Hunt & Reffert 2023 3.00 1.58 1.28 160 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2526 80.0 147.11 -51.3 0.29 -5.06 3.59 – 0.19

💡 Note: The % column shows the percentage of members that Theia 4371 shares with each listed object.

Visualization

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