HSC 2569

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0.35 UTI
0.26
CN
0.72
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.6 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.72 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2569 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate 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.

Palma et al. (2025)
Part of multiple system G160, along with HSC_2576 and NGC_5045.

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– 199.038 -63.385 0.476 -5.501 -1.359 -6.995
Hunt & Reffert 2024 199.092 -63.369 0.479 -5.518 -1.356 –
Cavallo et al. 2024 199.054 -63.399 0.48 – – –
Hunt & Reffert 2023 199.092 -63.369 0.479 -5.518 -1.356 –

💡 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– 2.015 1.365 0.58 198 0.240 166 – –
Hunt & Reffert 2024 – – – – – 166(1) – –
Cavallo et al. 2024 2.05 1.51 – 269 0.240 – – –
Hunt & Reffert 2023 1.98 1.22 0.58 127 – – – –

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

Visualization

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