Theia 7778

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0.19 UTI
0.0
CN
0.06
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 3.9 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 7778 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 311.726 35.708 0.444 -2.904 -4.218 –
Zhang et al. 2024 311.802 35.635 – – – –
Hunt & Reffert 2024 311.802 35.635 0.43 -2.859 -4.224 –
Cavallo et al. 2024 311.723 35.757 0.431 – – –
Hunt & Reffert 2023 311.802 35.635 0.43 -2.859 -4.224 –

💡 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] Bfrac BSS
UCC 99999– 2.1 0.81 0.65 219 -0.055 44 – –
Zhang et al. 2024 – – – – -0.310(1) – – –
Hunt & Reffert 2024 2.10 0.81 0.65 219 – 44(1) – –
Cavallo et al. 2024 2.29 0.93 – 123 0.200 – – –
Hunt & Reffert 2023 2.10 0.81 0.65 219 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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