Theia 398

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0.18 UTI
0.27
CN
0.39
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 18.8 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Theia 398 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, 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 Low extinction Low mass 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 – 104.04 -19.932 1.477 -5.317 1.506 25.878
Hunt & Reffert 2024 104.135 -19.922 1.494 -5.327 1.519 22.678
Cavallo et al. 2024 103.987 -19.738 1.491 – – –
Hunt & Reffert 2023 104.135 -19.922 1.494 -5.327 1.519 22.678

💡 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 – – – – – 48* – –
Cavallo et al. 2024 0.68 0.29 – 200 0.110 – – –
Hunt & Reffert 2023 0.65 0.11 0.68 129 – – – –

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

Visualization

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