HSC 2144

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0.32 UTI
0.37
CN
0.47
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.37 Poorly populated
  • Cdens 0.47 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2144 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.

Liu et al. (2025)
Classified as primordial binary cluster 62 along with CWNU_207.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P10, along with CWNU_207.

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 99999– 133.889 -45.437 1.156 -7.5 5.539 27.867
Cavallo et al. 2024 133.902 -45.503 1.186 – – –
Hunt & Reffert 2023 134.133 -45.418 1.165 -7.529 5.558 25.533

💡 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– 1.0 0.72 0.88 11 -0.310 – – –
Liu et al. 2025 1.05 0.33 – 17 – – – –
Cavallo et al. 2024 1.00 1.13 – 4 -0.310 – – –
Hunt & Reffert 2023 0.82 0.72 0.88 11 – – – –

Visualization

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