Theia 5504

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0.04 UTI
0.0
CN
0.07
Cdens
0.12
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 29.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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Theia 5504 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 23.589 57.112 1.088 1.651 -2.919 -12.502
Zhang et al. 2024 23.583 57.255 – – – –
Cavallo et al. 2024 22.567 57.076 1.094 – – –
Hunt & Reffert 2023 23.583 57.255 1.089 1.601 -2.969 -15.482

💡 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
Zhang et al. 2024 – – – – -0.043* – – –
Cavallo et al. 2024 0.90 0.80 – 269 0.050 – – –
Hunt & Reffert 2023 0.87 0.58 1.02 162 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 74 4.0 21.37 57.22 1.07 1.62 -2.98 -9.49 0.08

💡 Note: The % column shows the percentage of members that Theia 5504 shares with each listed object.

Visualization

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