HSC 1824

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0.30 UTI
0.41
CN
0.35
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 0.35 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1824 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Old

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 – 115.924 -13.356 0.204 -1.916 -1.001 55.523
Hu & Soubiran 2025 115.943 -13.373 – – – –
Hunt & Reffert 2024 115.909 -13.33 0.198 -1.911 -0.956 56.358
Cavallo et al. 2024 115.943 -13.373 0.204 – – –
Hunt & Reffert 2023 115.909 -13.33 0.198 -1.911 -0.956 56.358

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.200* – – –
Hunt & Reffert 2024 – – – – – 227* – –
Cavallo et al. 2024 3.98 1.14 – 2951 -0.430 – – –
Hunt & Reffert 2023 4.09 1.20 1.21 1503 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3226 85.4 115.92 -13.34 0.2 -1.92 -1.0 55.52 0.0

💡 Note: The % column shows the percentage of members that HSC 1824 shares with each listed object.

Visualization

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