Theia 850

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0.16 UTI
0.27
CN
0.17
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 30.8 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 850 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

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 Moderate extinction Near-solar metallicity Young

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 – 26.495 66.908 1.607 -5.599 -0.344 -19.939
Hunt & Reffert 2024 26.424 66.868 1.607 -5.577 -0.383 -21.8
Cavallo et al. 2024 25.413 67.123 1.6 – – –
Hunt & Reffert 2023 26.424 66.868 1.607 -5.577 -0.383 -21.8

💡 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 – – – – – 83* – –
Cavallo et al. 2024 0.68 1.93 – 24 0.060 – – –
Hunt & Reffert 2023 0.59 1.74 1.99 37 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4778 33.3 24.14 67.22 1.61 -5.68 -0.5 -23.51 0.08

💡 Note: The % column shows the percentage of members that Theia 850 shares with each listed object.

Visualization

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