HSC 2389

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0.50 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2389 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, 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.

Very distant Moderate extinction Massive 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 – 164.379 -59.733 0.166 -6.205 2.991 25.553
Hu & Soubiran 2025 164.382 -59.722 – – – –
Hunt & Reffert 2024 164.379 -59.727 0.163 -6.216 2.987 25.515
Cavallo et al. 2024 164.382 -59.722 0.165 – – –
Hunt & Reffert 2023 164.379 -59.727 0.163 -6.216 2.987 25.515

💡 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 – – – – – 1389* – –
Cavallo et al. 2024 8.20 2.93 – 759 -0.460 – – –
Hunt & Reffert 2023 5.61 2.82 1.75 1479 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3035 100.0 164.39 -59.74 0.15 -6.22 2.95 14.05 0.35

💡 Note: The % column shows the percentage of members that HSC 2389 shares with each listed object.

Visualization

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