Theia 283

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0.04 UTI
0.0
CN
0.11
Cdens
0.12
CC3
0.0
Clit
0.88
Cdup
Radius (P>50% members) 22.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

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Theia 283 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a relatively 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.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low extinction 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 – 109.042 -18.495 0.98 -3.399 4.049 8.959
Hunt & Reffert 2024 108.943 -18.58 0.948 -3.368 3.993 24.27
Cavallo et al. 2024 109.199 -18.659 0.951 – – –
Hunt & Reffert 2023 108.943 -18.58 0.948 -3.368 3.993 24.27

💡 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 – – – – – 70* – –
Cavallo et al. 2024 1.04 0.81 – 158 -0.300 – – –
Hunt & Reffert 2023 0.99 0.21 0.78 186 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 8 12.0 109.16 -18.98 1.04 -3.67 4.25 23.28 0.13

💡 Note: The % column shows the percentage of members that Theia 283 shares with each listed object.

Visualization

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