HSC 2110

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0.54 UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.7 [N/pc2]
  • CN 0.47 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 2110 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a large* distance, well below 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.

(*): The parallax distance estimate (~8.51 kpc) differs significantly from the median photometric distance (~6.12 kpc).

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– 122.797 -46.545 0.117 -2.576 4.415 78.358
Hu & Soubiran 2025 122.799 -46.541 – – – –
Hunt & Reffert 2024 122.792 -46.541 0.119 -2.584 4.368 71.644
Cavallo et al. 2024 122.799 -46.541 0.122 – – –
Hunt & Reffert 2023 122.792 -46.541 0.119 -2.584 4.368 71.644

💡 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– 6.12 1.175 1.04 1409 -0.355 536 – –
Hu & Soubiran 2025 – – – – -0.370(5) – – –
Hunt & Reffert 2024 – – – – – 536(1) – –
Cavallo et al. 2024 5.40 1.18 – 1778 -0.340 – – –
Hunt & Reffert 2023 6.84 1.17 1.04 1040 – – – –

(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 2974 100.0 122.8 -46.54 0.12 -2.56 4.42 78.36 0.3

💡 Note: The % column shows the percentage of members that HSC 2110 shares with each listed object.

Visualization

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