HSC 129

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0.39 UTI
0.31
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 11.0 [N/pc2]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 129 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Classified as optical pair P419, along with UFMG_75.

Cavallo et al. (2024)
Silver 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– 270.694 -19.766 0.364 0.694 -1.464 24.057
Hunt & Reffert 2024 270.683 -19.761 0.355 0.712 -1.418 24.058
Cavallo et al. 2024 270.676 -19.765 0.357 – – –
Hunt & Reffert 2023 270.683 -19.761 0.355 0.712 -1.418 24.058

💡 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– 2.535 4.805 2.65 102 0.080 1111 – –
Hunt & Reffert 2024 – – – – – 1111(1) – –
Cavallo et al. 2024 2.56 4.78 – 98 0.080 – – –
Hunt & Reffert 2023 2.51 4.83 2.65 106 – – – –

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

Visualization

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