HSC 131

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0.41 UTI
0.3
CN
0.52
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.52 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 131 is a poorly populated, moderately dense 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, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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– 275.131 -22.024 1.29 1.82 -0.127 -10.049
Hu & Soubiran 2025 275.102 -22.004 – – – –
Hunt & Reffert 2024 274.987 -21.895 1.254 1.753 -0.058 -6.576
Cavallo et al. 2024 275.102 -22.004 1.262 – – –
Hunt & Reffert 2023 274.987 -21.895 1.254 1.753 -0.058 -6.576

💡 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– 0.72 0.805 1.1 390 -0.195 167 – –
Hu & Soubiran 2025 – – – – -0.260(5) – – –
Hunt & Reffert 2024 – – – – – 167(1) – –
Cavallo et al. 2024 0.69 0.79 – 617 -0.130 – – –
Hunt & Reffert 2023 0.75 0.82 1.10 163 – – – –

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

Visualization

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