Theia 3862

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0.15 UTI
0.0
CN
0.1
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 25.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Theia 3862 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close 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.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Moderate 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 – 33.173 57.851 1.1 3.386 -3.781 -2.436
Zhang et al. 2024 33.169 57.839 – – – –
Cavallo et al. 2024 32.232 58.102 1.066 – – –
Hunt & Reffert 2023 33.169 57.839 1.068 3.427 -3.731 -17.601

💡 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 – – – – -0.082* – – –
Cavallo et al. 2024 0.96 1.34 – 132 0.180 – – –
Hunt & Reffert 2023 0.89 0.95 0.73 119 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4145 80.0 32.81 58.02 1.09 3.38 -3.77 -16.37 0.03

💡 Note: The % column shows the percentage of members that Theia 3862 shares with each listed object.

Visualization

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