Theia 3823

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0.20 UTI
0.56
CN
1.0
Cdens
0.5
CC3
0.0
Clit
0.48
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.48 Possibly duplicate

Overview

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Theia 3823 is a moderately populated, very 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, young 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 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 – 142.75 -50.305 0.662 -6.352 5.667 23.023
Hunt & Reffert 2024 142.761 -50.314 0.664 -6.368 5.66 –
Cavallo et al. 2024 142.768 -50.319 0.667 – – –
Hunt & Reffert 2023 142.761 -50.314 0.664 -6.368 5.66 –

💡 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 – – – – – 299* – –
Cavallo et al. 2024 1.43 2.37 – 72 -0.230 – – –
Hunt & Reffert 2023 1.43 1.96 2.27 81 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1459 51.6 142.76 -50.31 0.66 -6.33 5.63 – 0.34

💡 Note: The % column shows the percentage of members that Theia 3823 shares with each listed object.

Visualization

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