Theia 1754

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0.03 UTI
0.56
CN
0.34
Cdens
1.0
CC3
0.03
Clit
0.06
Cdup
Core radius and density 1.8 [pc], 1.7 [pc-2]
  • CN 0.56 Moderately populated
  • Cdens 0.34 Loose
  • CC3 1.0 Very high quality
  • Clit 0.03 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

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Theia 1754 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-rich, 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.97 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (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– 295.703 23.698 0.55 -1.781 -4.22 27.398
Hunt & Reffert 2024 295.689 23.653 0.547 -1.788 -4.218 27.701
Cavallo et al. 2024 295.709 23.694 0.55 – – –
Hunt & Reffert 2023 295.689 23.653 0.547 -1.788 -4.218 27.701

💡 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– 1.75 2.47 1.77 75 1.050 343 – –
Hunt & Reffert 2024 1.75 2.47 1.77 75 – 343(1) – –
Cavallo et al. 2024 2.05 2.06 – 151 1.050 – – –
Hunt & Reffert 2023 1.75 2.47 1.77 75 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
PHOC 13 93.5 295.7 23.7 0.54 -1.77 -4.23 27.71 0.4

💡 Note: The % column shows the percentage of members that Theia 1754 shares with each listed object.

Visualization

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