Theia 2103

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0.19 UTI
0.26
CN
0.19
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 23.2 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.19 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 2103 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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 Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 121.382 -40.944 1.306 -4.467 3.834 33.806
Hunt & Reffert 2024 121.385 -40.943 1.311 -4.471 3.824 31.18
Cavallo et al. 2024 121.271 -40.812 1.312 – – –
Hunt & Reffert 2023 121.385 -40.943 1.311 -4.471 3.824 31.18

💡 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 – – – – – 75* – –
Cavallo et al. 2024 0.88 0.49 – 105 0.320 – – –
Hunt & Reffert 2023 0.74 0.55 0.67 29 – – – –

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

Visualization

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