Theia 1886

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0.30 UTI
0.4
CN
0.86
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.86 Dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 1886 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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 large percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Near-solar metallicity 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 – 246.685 -49.165 0.362 -1.737 -2.447 -58.675
Hunt & Reffert 2024 246.663 -49.145 0.366 -1.733 -2.425 -45.527
Cavallo et al. 2024 246.712 -49.16 0.366 – – –
Hunt & Reffert 2023 246.663 -49.145 0.366 -1.733 -2.425 -45.527

💡 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 – – – – – 759* – –
Cavallo et al. 2024 2.21 3.44 – 58 0.290 – – –
Hunt & Reffert 2023 2.50 3.46 2.44 33 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3800 92.5 246.71 -49.17 0.37 -1.74 -2.44 -58.68 0.07

💡 Note: The % column shows the percentage of members that Theia 1886 shares with each listed object.

Visualization

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