Theia 1806

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0.06 UTI
0.34
CN
1.0
Cdens
0.12
CC3
0.25
Clit
0.15
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.15 Likely duplicate

Overview

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Theia 1806 is a poorly populated, very dense object of very low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate 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 – 85.449 27.492 0.758 -0.325 -4.367 -2.946
Hu & Soubiran 2025 85.409 27.458 – – – –
Hunt & Reffert 2024 85.433 27.5 0.734 -0.208 -4.369 -3.067
Cavallo et al. 2024 85.409 27.458 0.737 – – –
Hunt & Reffert 2023 85.433 27.5 0.734 -0.208 -4.369 -3.067

💡 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 – – – – -0.200* – – –
Hunt & Reffert 2024 – – – – – 176* – –
Cavallo et al. 2024 1.50 1.51 – 513 0.360 – – –
Hunt & Reffert 2023 1.28 1.79 2.39 187 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 127 85.3 85.44 27.48 0.76 -0.34 -4.36 7.82 0.3

💡 Note: The % column shows the percentage of members that Theia 1806 shares with each listed object.

Visualization

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