HSC 2550

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0.38 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2550 is a sparse, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near 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.

Liu et al. (2025)
Classified as primordial binary cluster 236 along with OC_0587, and of multiple system 27 along with OC_0587 and CWNU_490.

Palma et al. (2025)
Part of multiple system G159, along with CWNU_490 and OC_0587.

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– 195.106 -62.381 0.507 -5.079 -1.79 –
Liu et al. 2025 195.11 -62.4 0.52 -5.09 -1.78 –
Hunt & Reffert 2024 195.108 -62.397 0.516 -5.092 -1.784 –
Cavallo et al. 2024 195.089 -62.405 0.514 – – –
Hunt & Reffert 2023 195.108 -62.397 0.516 -5.092 -1.784 –

💡 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– 1.84 2.23 1.86 25 -0.370 368 – –
Liu et al. 2025 4.27 0.81 – 25 – – – –
Hunt & Reffert 2024 – – – – – 368(1) – –
Cavallo et al. 2024 1.70 2.49 – 37 -0.370 – – –
Hunt & Reffert 2023 1.84 2.23 1.86 15 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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