Theia 3423

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0.03 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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Theia 3423 is a sparse, very dense 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 an old cluster (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 Old

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 124.7 -30.585 0.585 -3.019 2.626 –
Hunt & Reffert 2024 124.677 -30.562 0.749 -3.039 2.646 49.708
Hunt & Reffert 2023 124.677 -30.562 0.749 -3.039 2.646 49.708

💡 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 – – – – – 106* – –
Hunt & Reffert 2023 1.32 0.23 0.37 1738 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Melotte 86 88.0 124.64 -30.62 0.57 -2.97 2.61 34.59 0.96

💡 Note: The % column shows the percentage of members that Theia 3423 shares with each listed object.

Visualization

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