HSC 2116

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0.35 UTI
0.32
CN
0.17
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.17 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2116 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a large distance, well 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.

Very 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 – 137.404 -39.221 0.162 -4.04 3.715 85.126
Hu & Soubiran 2025 137.378 -39.182 – – – –
Hunt & Reffert 2024 137.402 -39.203 0.162 -4.026 3.671 91.268
Cavallo et al. 2024 137.378 -39.182 0.159 – – –
Hunt & Reffert 2023 137.402 -39.203 0.162 -4.026 3.671 91.268

💡 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 – – – – -0.190* – – –
Hunt & Reffert 2024 – – – – – 268* – –
Cavallo et al. 2024 5.18 1.07 – 1549 -0.200 – – –
Hunt & Reffert 2023 5.48 1.33 0.87 897 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3281 100.0 137.41 -39.23 0.16 -4.03 3.68 89.55 0.17

💡 Note: The % column shows the percentage of members that HSC 2116 shares with each listed object.

Visualization

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