Theia 1813

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0.08 UTI
0.68
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.13
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.13 Likely duplicate

Overview

â„šī¸
Theia 1813 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, 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.

Distant High extinction Massive Metal-poor 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 – 264.34 -33.842 0.244 -0.889 -2.067 -4.184
Hu & Soubiran 2025 264.324 -33.839 – – – –
Hunt & Reffert 2024 264.338 -33.838 0.255 -0.883 -2.075 -5.053
Cavallo et al. 2024 264.324 -33.839 0.254 – – –
Hunt & Reffert 2023 264.338 -33.838 0.255 -0.883 -2.075 -5.053

💡 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 – – – – -0.410* – – –
Hunt & Reffert 2024 – – – – – 3928* – –
Cavallo et al. 2024 6.14 4.44 – 631 -1.220 – – –
Hunt & Reffert 2023 3.41 4.71 2.31 330 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1200 87.2 264.34 -33.84 0.24 -0.85 -2.06 -3.9 0.54

💡 Note: The % column shows the percentage of members that Theia 1813 shares with each listed object.

Visualization

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