Theia 2052

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0.05 UTI
0.25
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.25 Poorly populated
  • 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 2052 is a poorly populated, 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.

Relatively close Moderate extinction Metal-poor 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 – 250.941 -47.094 0.357 -2.991 -4.21 -43.786
Hunt & Reffert 2024 250.946 -47.089 0.366 -2.93 -4.18 -39.942
Cavallo et al. 2024 250.949 -47.095 0.367 – – –
Hunt & Reffert 2023 250.946 -47.089 0.366 -2.93 -4.18 -39.942

💡 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 – – – – – 255* – –
Cavallo et al. 2024 1.89 2.02 – 93 -0.870 – – –
Hunt & Reffert 2023 2.62 1.50 0.39 110 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1552 88.0 250.94 -47.09 0.35 -2.96 -4.22 – 0.45

💡 Note: The % column shows the percentage of members that Theia 2052 shares with each listed object.

Visualization

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