Theia 3716

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0.17 UTI
0.32
CN
0.09
Cdens
0.75
CC3
0.03
Clit
0.69
Cdup
Core radius and density 2.4 [pc], 0.4 [pc-2]
  • CN 0.32 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.75 High quality
  • Clit 0.03 Rarely studied
  • Cdup 0.69 Likely unique

Overview

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Theia 3716 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near 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.

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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 8.775 63.003 0.345 -2.984 -0.596 –
Hunt & Reffert 2024 8.751 62.983 0.345 -2.987 -0.591 –
Cavallo et al. 2024 8.726 63.003 0.345 – – –
Hunt & Reffert 2023 8.751 62.983 0.345 -2.987 -0.591 –

💡 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] Bfrac BSS
UCC 99999– 2.67 1.35 0.76 89 -0.240 343 – –
Hunt & Reffert 2024 2.67 1.35 0.76 89 – 343(1) – –
Cavallo et al. 2024 2.41 1.32 – 141 -0.240 – – –
Hunt & Reffert 2023 2.67 1.35 0.76 89 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3091 100.0 8.78 63.02 0.35 -2.97 -0.58 – 0.12
FoF 1864 31.2 8.7 63.04 0.35 -2.91 -0.56 – 0.07

💡 Note: The % column shows the percentage of members that Theia 3716 shares with each listed object.

Visualization

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