Theia 3739

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0.02 UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.0
Clit
0.06
Cdup
Stellar density (N50/rad) 13.6 [N/pc2]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

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Theia 3739 is a poorly populated, very dense object of intermediate 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, intermediate-age 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.

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 99999– 15.952 61.893 0.411 -0.265 0.163 4.797
Hunt & Reffert 2024 15.968 61.892 0.403 -0.277 0.142 4.797
Cavallo et al. 2024 15.924 61.895 0.409 – – –
Hunt & Reffert 2023 15.968 61.892 0.403 -0.277 0.142 4.797

💡 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– 2.275 2.415 1.15 372 0.240 254 – –
Hunt & Reffert 2024 – – – – – 254(1) – –
Cavallo et al. 2024 2.31 2.37 – 407 0.240 – – –
Hunt & Reffert 2023 2.24 2.46 1.15 337 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1213 93.9 15.95 61.89 0.41 -0.28 0.17 4.8 0.36

💡 Note: The % column shows the percentage of members that Theia 3739 shares with each listed object.

Visualization

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