Theia 2406

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0.26 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.43
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.43 Possibly duplicate

Overview

â„šī¸
Theia 2406 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Low 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 – 117.42 -26.846 0.211 -2.081 2.768 100.313
Hu & Soubiran 2025 117.419 -26.842 – – – –
Hunt & Reffert 2024 117.416 -26.844 0.209 -2.082 2.772 106.499
Cavallo et al. 2024 117.419 -26.842 0.211 – – –
Hunt & Reffert 2023 117.416 -26.844 0.209 -2.082 2.772 106.499

💡 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
Hu & Soubiran 2025 – – – – -0.240* – – –
Hunt & Reffert 2024 – – – – – 960* – –
Cavallo et al. 2024 3.61 0.83 – 724 0.140 – – –
Hunt & Reffert 2023 4.08 0.83 1.83 450 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 639 57.1 117.42 -26.84 0.2 -2.08 2.75 94.96 0.5

💡 Note: The % column shows the percentage of members that Theia 2406 shares with each listed object.

Visualization

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