Theia 3381

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0.35 UTI
0.38
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 3381 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a very small percentage of members with a later 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 – 203.679 -63.335 0.468 -3.817 -1.635 –
Hunt & Reffert 2024 203.684 -63.334 0.456 -3.878 -1.584 –
Cavallo et al. 2024 203.298 -63.316 0.458 – – –
Hunt & Reffert 2023 203.684 -63.334 0.456 -3.878 -1.584 –

💡 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 – – – – – 66* – –
Cavallo et al. 2024 1.82 1.30 – 11 -0.020 – – –
Hunt & Reffert 2023 1.98 1.22 2.16 31 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3722 5.3 204.14 -63.64 0.45 -3.62 -1.71 6.7 0.13

💡 Note: The % column shows the percentage of members that Theia 3381 shares with each listed object.

Visualization

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