Theia 2325

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0.13 UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.27
Cdup
Radius (P>50% members) 9.1 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.27 Possibly duplicate

Overview

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Theia 2325 is a moderately populated, very dense object of high 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 (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.

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 – 223.139 -61.503 0.931 -2.241 -1.859 0.626
Hunt & Reffert 2024 223.114 -61.49 0.934 -2.243 -1.887 14.089
Cavallo et al. 2024 223.243 -61.468 0.936 – – –
Hunt & Reffert 2023 223.114 -61.49 0.934 -2.243 -1.887 14.089

💡 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 – – – – – 393* – –
Cavallo et al. 2024 1.00 2.18 – 117 -0.260 – – –
Hunt & Reffert 2023 1.01 1.83 2.27 97 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2312 73.0 223.14 -61.49 0.93 -2.25 -1.86 12.66 0.55
OC 0616 43.2 223.14 -61.47 0.93 -2.27 -1.86 23.94 0.0

💡 Note: The % column shows the percentage of members that Theia 2325 shares with each listed object.

Visualization

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