Theia 1450

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0.23 UTI
0.38
CN
0.42
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 18.5 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.42 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 1450 is a poorly populated, 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, intermediate-age 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 Moderate extinction Near-solar metallicity Intermediate age

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 – 315.201 49.778 1.259 5.91 2.998 -49.982
Hunt & Reffert 2024 315.494 49.824 1.26 5.887 3.127 -49.531
Cavallo et al. 2024 314.338 49.449 1.262 – – –
Hunt & Reffert 2023 315.494 49.824 1.26 5.887 3.127 -49.531

💡 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 – – – – – 74* – –
Cavallo et al. 2024 0.91 2.59 – 263 0.460 – – –
Hunt & Reffert 2023 0.75 3.14 2.78 223 – – – –

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

Visualization

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