Theia 3202

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0.05 UTI
0.34
CN
0.6
Cdens
0.5
CC3
0.25
Clit
0.12
Cdup
Radius (P>50% members) 8.8 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.6 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 0.12 Likely duplicate

Overview

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Theia 3202 is a poorly populated, moderately dense object of intermediate 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)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 309.879 38.537 0.762 -0.19 -0.73 -2.711
Zhang et al. 2024 309.861 38.486 – – – –
Hunt & Reffert 2024 309.861 38.486 0.745 -0.131 -0.539 2.22
Cavallo et al. 2024 310.458 38.832 0.747 – – –
Hunt & Reffert 2023 309.861 38.486 0.745 -0.131 -0.539 2.22

💡 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 – – – – 0.203* – – –
Hunt & Reffert 2024 – – – – – 131* – –
Cavallo et al. 2024 1.44 2.91 – 309 -0.250 – – –
Hunt & Reffert 2023 1.29 2.57 2.49 213 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 478 88.2 309.96 38.58 0.77 -0.21 -0.74 -2.71 0.35

💡 Note: The % column shows the percentage of members that Theia 3202 shares with each listed object.

Visualization

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