Theia 5724

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0.14 UTI
0.37
CN
0.72
Cdens
1.0
CC3
0.0
Clit
0.32
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 0.72 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

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Theia 5724 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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.

Relatively close Moderate extinction Metal-rich 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 – 297.402 29.089 0.29 -1.424 -4.564 –
Hunt & Reffert 2024 297.393 29.086 0.295 -1.421 -4.554 3.134
Cavallo et al. 2024 297.381 29.076 0.296 – – –
Hunt & Reffert 2023 297.393 29.086 0.295 -1.421 -4.554 3.134

💡 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 – – – – – 444* – –
Cavallo et al. 2024 2.90 1.61 – 302 0.540 – – –
Hunt & Reffert 2023 2.89 1.66 1.67 131 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1071 67.6 297.39 29.08 0.3 -1.42 -4.56 – 0.45

💡 Note: The % column shows the percentage of members that Theia 5724 shares with each listed object.

Visualization

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