Theia 2231

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0.05 UTI
0.0
CN
0.26
Cdens
0.38
CC3
0.25
Clit
0.24
Cdup
Radius (P>50% members) 7.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.26 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.24 Likely duplicate

Overview

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Theia 2231 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above 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 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 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 – 90.119 27.673 0.589 0.146 -2.113 –
Zhang et al. 2024 90.135 27.686 – – – –
Hunt & Reffert 2024 90.135 27.686 0.586 0.177 -2.097 –
Cavallo et al. 2024 90.124 27.694 0.587 – – –
Hunt & Reffert 2023 90.135 27.686 0.586 0.177 -2.097 –

💡 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
Zhang et al. 2024 – – – – -0.239* – – –
Hunt & Reffert 2024 – – – – – 117* – –
Cavallo et al. 2024 1.68 0.88 – 74 0.190 – – –
Hunt & Reffert 2023 1.62 0.81 0.52 133 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 516 76.0 90.11 27.68 0.59 0.15 -2.1 – 0.14

💡 Note: The % column shows the percentage of members that Theia 2231 shares with each listed object.

Visualization

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