Theia 1756

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0.41 UTI
0.76
CN
0.65
Cdens
0.75
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 6.5 [arcmin]
  • CN 0.76 Rich
  • Cdens 0.65 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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Theia 1756 is a rich, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

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

Relatively close High extinction Very massive Near-solar metallicity Young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 274.017 -16.404 0.313 -0.499 -2.121 14.968
Hunt & Reffert 2024 274.02 -16.41 0.325 -0.467 -2.085 34.36
Cavallo et al. 2024 273.895 -16.5 0.325 – – –
Hunt & Reffert 2023 274.02 -16.41 0.325 -0.467 -2.085 34.36

💡 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 – – – – – 5692* – –
Cavallo et al. 2024 3.06 4.65 – 19 0.120 – – –
Hunt & Reffert 2023 2.78 3.75 3.19 92 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2798 4.2 274.01 -16.47 0.32 -0.77 -2.55 30.15 0.44
Ryu 212 3.4 274.21 -16.31 0.33 -0.36 -2.39 -0.92 0.31

💡 Note: The % column shows the percentage of members that Theia 1756 shares with each listed object.

Visualization

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