Theia 7478

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0.20 UTI
0.26
CN
0.26
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 17.4 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.26 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 7478 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, below 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 – 312.541 33.679 1.123 3.098 -1.67 -4.585
Zhang et al. 2024 312.765 33.806 – – – –
Cavallo et al. 2024 312.436 33.71 1.119 – – –
Hunt & Reffert 2023 312.765 33.806 1.092 3.207 -1.659 -5.556

💡 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 – – – – -0.094* – – –
Cavallo et al. 2024 0.85 0.49 – 170 -0.120 – – –
Hunt & Reffert 2023 0.86 0.17 0.33 172 – – – –

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

Visualization

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