HSC 2817

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0.36 UTI
0.0
CN
0.79
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.79 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2817 is a sparse, dense object of intermediate 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, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It was recently reported in the literature.

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– 252.771 -47.05 1.309 -1.79 -6.38 -5.228
Hu & Soubiran 2025 252.896 -46.903 – – – –
Hunt & Reffert 2024 252.761 -47.118 1.301 -1.798 -6.343 -1.694
Cavallo et al. 2024 252.896 -46.903 1.298 – – –
Hunt & Reffert 2023 252.761 -47.118 1.301 -1.798 -6.343 -1.694

💡 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– 0.75 0.385 0.64 298 0.050 64 – –
Hu & Soubiran 2025 – – – – -0.110(5) – – –
Hunt & Reffert 2024 – – – – – 64(1) – –
Cavallo et al. 2024 0.77 0.17 – 513 0.210 – – –
Hunt & Reffert 2023 0.73 0.60 0.64 83 – – – –

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

Visualization

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