Theia 2133

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0.33 UTI
0.37
CN
0.18
Cdens
0.75
CC3
0.25
Clit
0.92
Cdup
Radius (P>50% members) 10.5 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 0.18 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.92 Very likely unique

Overview

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Theia 2133 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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 – 98.291 12.425 0.471 -0.358 -0.91 -1.284
Zhang et al. 2024 98.287 12.438 – – – –
Hunt & Reffert 2024 98.287 12.438 0.475 -0.344 -0.955 -1.282
Cavallo et al. 2024 98.285 12.184 0.478 – – –
Hunt & Reffert 2023 98.287 12.438 0.475 -0.344 -0.955 -1.282

💡 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 – – – – -0.360* – – –
Hunt & Reffert 2024 – – – – – 195* – –
Cavallo et al. 2024 2.00 1.59 – 26 0.130 – – –
Hunt & Reffert 2023 1.91 1.45 2.31 67 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2535 8.1 98.35 11.96 0.48 -0.34 -0.98 46.02 0.2

💡 Note: The % column shows the percentage of members that Theia 2133 shares with each listed object.

Visualization

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