Theia 4930

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0.23 UTI
0.29
CN
0.24
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 18.2 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.24 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 4930 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, 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 Low mass 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 – 124.372 -36.733 1.071 -6.08 4.881 32.682
Hunt & Reffert 2024 124.383 -36.676 1.067 -6.102 4.893 35.423
Cavallo et al. 2024 124.403 -36.739 1.074 – – –
Hunt & Reffert 2023 124.383 -36.676 1.067 -6.102 4.893 35.423

💡 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 – – – – – 40* – –
Cavallo et al. 2024 0.94 1.04 – 62 -0.120 – – –
Hunt & Reffert 2023 0.90 0.21 0.83 250 – – – –

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

Visualization

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