Theia 1858

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0.16 UTI
0.75
CN
0.75
Cdens
0.75
CC3
0.0
Clit
0.36
Cdup
Radius (P>50% members) 16.0 [arcmin]
  • CN 0.75 Rich
  • Cdens 0.75 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

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Theia 1858 is a rich, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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 Metal-rich 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 – 135.75 -46.727 0.87 -6.089 3.987 8.702
Hunt & Reffert 2024 135.734 -46.726 0.854 -6.045 3.961 19.058
Cavallo et al. 2024 135.676 -46.698 0.856 – – –
Hunt & Reffert 2023 135.734 -46.726 0.854 -6.045 3.961 19.058

💡 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 – – – – – 476* – –
Cavallo et al. 2024 1.32 2.85 – 41 0.690 – – –
Hunt & Reffert 2023 1.12 2.96 2.72 29 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14384 63.9 135.76 -46.73 0.87 -6.11 4.01 12.22 0.26
OC 0496 25.9 135.71 -46.74 0.87 -6.08 4.02 26.5 0.28
CWNU 188 23.1 135.69 -46.73 0.88 -6.11 4.01 26.5 0.04

💡 Note: The % column shows the percentage of members that Theia 1858 shares with each listed object.

Visualization

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