Theia 648

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0.07 UTI
0.0
CN
0.11
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 33.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 648 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close 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.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 86.58 25.973 1.669 1.035 -3.212 -7.453
Zhang et al. 2024 86.578 25.965 – – – –
Cavallo et al. 2024 86.306 26.191 1.724 – – –
Hunt & Reffert 2023 86.578 25.965 1.724 1.099 -3.153 -4.66

💡 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
Zhang et al. 2024 – – – – 0.000* – – –
Cavallo et al. 2024 0.58 0.43 – 186 0.140 – – –
Hunt & Reffert 2023 0.55 0.51 0.34 130 – – – –

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

Visualization

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