HSC 56

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0.39 UTI
0.46
CN
1.0
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 6.0 [N/pc2]
  • CN 0.46 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 56 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 high extinction. It is catalogued as a massive, metal-poor, young cluster (see Parameters). It was recently reported in the literature.

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

Palma et al. (2025)
Part of multiple system G183, along with UBC_93 and CWNU_2379.

Cavallo et al. (2024)
Bronze 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– 268.435 -25.108 0.327 -0.233 -2.118 -5.149
Hunt & Reffert 2024 268.429 -25.105 0.324 -0.257 -2.127 94.495
Cavallo et al. 2024 268.448 -25.115 0.322 – – –
Hunt & Reffert 2023 268.429 -25.105 0.324 -0.257 -2.127 94.495

💡 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– 2.495 4.775 2.88 32 -0.880 1831 – –
Hunt & Reffert 2024 – – – – – 1831(1) – –
Cavallo et al. 2024 2.12 5.25 – 11 -0.880 – – –
Hunt & Reffert 2023 2.87 4.30 2.88 54 – – – –

(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 4088 58.7 268.44 -25.11 0.32 -0.17 -2.09 102.64 0.06

💡 Note: The % column shows the percentage of members that HSC 56 shares with each listed object.

Visualization

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