Theia 153

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0.17 UTI
0.33
CN
0.41
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 16.3 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.41 Loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 153 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a close distance, near 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.

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 – 355.941 60.167 1.184 -1.59 -1.928 -7.894
Hunt & Reffert 2024 355.942 60.133 1.177 -1.581 -1.944 -7.819
Cavallo et al. 2024 356.206 60.246 1.181 – – –
Hunt & Reffert 2023 355.942 60.133 1.177 -1.581 -1.944 -7.819

💡 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 – – – – – 79* – –
Cavallo et al. 2024 0.90 1.89 – 24 0.030 – – –
Hunt & Reffert 2023 0.81 1.67 2.07 34 – – – –

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

Visualization

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