Theia 2145

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0.15 UTI
0.0
CN
0.53
Cdens
0.25
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 2.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.53 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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Theia 2145 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very 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=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate 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 – 145.786 -54.298 0.236 -4.598 3.013 –
Hunt & Reffert 2024 145.803 -54.3 0.232 -4.605 3.007 32.412
Cavallo et al. 2024 145.934 -54.311 0.233 – – –
Hunt & Reffert 2023 145.803 -54.3 0.232 -4.605 3.007 32.412

💡 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 – – – – – 387* – –
Cavallo et al. 2024 3.56 1.81 – 417 0.400 – – –
Hunt & Reffert 2023 4.08 2.17 2.19 151 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4766 92.0 145.79 -54.3 0.24 -4.6 3.01 – 0.07
CWWDL 5026 4.0 145.79 -54.33 0.29 -4.64 3.17 25.75 0.06

💡 Note: The % column shows the percentage of members that Theia 2145 shares with each listed object.

Visualization

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