HSC 2320

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0.35 UTI
0.36
CN
1.0
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 5.9 [N/pc2]
  • CN 0.36 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2320 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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.

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– 151.329 -59.186 0.177 -5.112 2.677 –
Hunt & Reffert 2024 151.328 -59.185 0.186 -5.116 2.686 –
Cavallo et al. 2024 151.335 -59.184 0.184 – – –
Hunt & Reffert 2023 151.328 -59.185 0.186 -5.116 2.686 –

💡 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– 4.41 2.205 1.62 214 0.560 692 – –
Hunt & Reffert 2024 – – – – – 692(1) – –
Cavallo et al. 2024 3.94 1.86 – 380 0.560 – – –
Hunt & Reffert 2023 4.88 2.55 1.62 49 – – – –

(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 3189 100.0 151.33 -59.18 0.17 -5.11 2.68 – 0.06

💡 Note: The % column shows the percentage of members that HSC 2320 shares with each listed object.

Visualization

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