HSC 2824

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0.30 UTI
0.43
CN
0.3
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2824 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

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

Palma et al. (2025)
Part of multiple system G97, along with Theia_1891, NGC_6249 and Harvard_13.

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– 255.237 -46.713 0.825 1.508 -3.799 -38.066
Hunt & Reffert 2024 255.206 -46.682 0.823 1.4 -3.854 -23.78
Cavallo et al. 2024 255.391 -47.064 0.825 – – –
Hunt & Reffert 2023 255.206 -46.682 0.823 1.4 -3.854 -23.78

💡 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– 1.25 3.2 2.75 16 0.230 166 – –
Hunt & Reffert 2024 – – – – – 166(1) – –
Cavallo et al. 2024 1.35 3.23 – 10 0.230 – – –
Hunt & Reffert 2023 1.15 3.17 2.75 23 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4183 44.2 255.22 -46.94 0.82 1.43 -3.82 -38.07 0.02

💡 Note: The % column shows the percentage of members that HSC 2824 shares with each listed object.

Visualization

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