HSC 2368

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0.27 UTI
0.0
CN
0.35
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.35 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2368 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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 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.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 152 along with FoF_403.

Palma et al. (2025)
Part of multiple system G78, along with Theia_2185 and LP_403.

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– 162.103 -58.025 0.378 -7.094 2.818 –
Hunt & Reffert 2024 162.154 -58.034 0.375 -7.097 2.816 –
Cavallo et al. 2024 162.126 -58.027 0.373 – – –
Hunt & Reffert 2023 162.154 -58.034 0.375 -7.097 2.816 –

💡 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– 3.22 2.22 1.08 29 0.230 176 – –
Liu et al. 2025 5.20 0.72 – 71 – – – –
Hunt & Reffert 2024 – – – – – 176(1) – –
Cavallo et al. 2024 3.22 2.22 – 29 0.230 – – –
Hunt & Reffert 2023 2.52 2.29 1.08 22 – – – –

(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 4621 88.0 162.1 -58.0 0.37 -7.09 2.83 – 0.02

💡 Note: The % column shows the percentage of members that HSC 2368 shares with each listed object.

Visualization

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