Theia 7057

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0.22 UTI
0.0
CN
0.36
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.36 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 7057 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low 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 – 116.18 -25.396 0.323 -2.771 4.439 –
Hunt & Reffert 2024 116.173 -25.365 0.304 -2.769 4.451 69.838
Cavallo et al. 2024 116.218 -25.396 0.31 – – –
Hunt & Reffert 2023 116.173 -25.365 0.304 -2.769 4.451 69.838

💡 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 – – – – – 117* – –
Cavallo et al. 2024 3.09 0.88 – 162 0.090 – – –
Hunt & Reffert 2023 2.73 0.50 0.88 470 – – – –

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

Visualization

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