Theia 3857

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0.23 UTI
0.32
CN
0.43
Cdens
1.0
CC3
0.0
Clit
0.66
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.43 Loose
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.66 Likely unique

Overview

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Theia 3857 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

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

Distant High extinction Massive Metal-rich Very young

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 – 233.38 -58.655 0.308 -3.397 -3.57 8.788
Hunt & Reffert 2024 233.382 -58.658 0.303 -3.418 -3.573 112.75
Cavallo et al. 2024 233.173 -58.587 0.303 – – –
Hunt & Reffert 2023 233.382 -58.658 0.303 -3.418 -3.573 112.75

💡 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 – – – – – 1154* – –
Cavallo et al. 2024 4.25 3.51 – 7 0.500 – – –
Hunt & Reffert 2023 3.17 3.56 2.80 11 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2248 34.4 233.66 -58.55 0.31 -3.37 -3.51 -55.84 0.11

💡 Note: The % column shows the percentage of members that Theia 3857 shares with each listed object.

Visualization

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