Theia 8106

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0.03 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.08
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.08 Very likely duplicate

Overview

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Theia 8106 is a sparse, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 very 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 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 – 137.356 -43.318 0.391 -4.439 4.985 –
Hunt & Reffert 2024 137.359 -43.309 0.396 -4.417 4.942 –
Cavallo et al. 2024 137.331 -43.411 0.401 – – –
Hunt & Reffert 2023 137.359 -43.309 0.396 -4.417 4.942 –

💡 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 – – – – – 122* – –
Cavallo et al. 2024 2.58 2.24 – 17 0.060 – – –
Hunt & Reffert 2023 2.29 2.06 2.18 48 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0490 92.0 137.36 -43.32 0.4 -4.44 4.99 – 0.3

💡 Note: The % column shows the percentage of members that Theia 8106 shares with each listed object.

Visualization

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