HSC 87

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0.56 UTI
0.3
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.3 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 87 is a poorly populated, very dense object of very high 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, 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– 272.564 -25.064 0.884 1.501 0.503 33.846
Hu & Soubiran 2025 272.567 -25.045 – – – –
Hunt & Reffert 2024 272.505 -25.091 0.862 1.498 0.523 20.869
Cavallo et al. 2024 272.567 -25.045 0.862 – – –
Hunt & Reffert 2023 272.505 -25.091 0.862 1.498 0.523 20.869

💡 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– 1.18 1.22 0.42 568 -0.480 155 – –
Hu & Soubiran 2025 – – – – -0.230(5) – – –
Hunt & Reffert 2024 – – – – – 155(1) – –
Cavallo et al. 2024 1.27 1.65 – 1000 -0.730 – – –
Hunt & Reffert 2023 1.09 0.79 0.42 137 – – – –

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

Visualization

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