HSC 1462

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0.20 UTI
0.0
CN
0.16
Cdens
0.25
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.25 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1462 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity 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– 87.281 23.96 1.163 2.313 -4.67 8.875
Hu & Soubiran 2025 87.33 23.897 – – – –
Zhang et al. 2024 87.173 23.992 – – – –
Hunt & Reffert 2024 87.173 23.992 1.172 2.336 -4.624 8.551
Cavallo et al. 2024 87.33 23.897 1.171 – – –
Hunt & Reffert 2023 87.173 23.992 1.172 2.336 -4.624 8.551

💡 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– 0.825 0.43 0.45 540 -0.160 40 – –
Hu & Soubiran 2025 – – – – -0.220(5) – – –
Zhang et al. 2024 – – – – -0.160(1) – – –
Hunt & Reffert 2024 – – – – – 40(1) – –
Cavallo et al. 2024 0.85 0.43 – 724 0.380 – – –
Hunt & Reffert 2023 0.80 0.43 0.45 357 – – – –

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

Visualization

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