HSC 2350

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0.42 UTI
0.57
CN
0.29
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 0.29 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2350 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a very 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.

(*): The parallax distance estimate (~12.84 kpc) differs significantly from the median photometric distance (~7.79 kpc).

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 – 161.957 -55.867 0.078 -4.243 2.016 52.173
Hu & Soubiran 2025 161.94 -55.865 – – – –
Hunt & Reffert 2024 161.956 -55.878 0.092 -4.292 2.029 52.479
Cavallo et al. 2024 161.94 -55.865 0.094 – – –
Hunt & Reffert 2023 161.956 -55.878 0.092 -4.292 2.029 52.479

💡 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 – – – – -0.210* – – –
Hunt & Reffert 2024 – – – – – 829* – –
Cavallo et al. 2024 7.28 1.89 – 2399 0.090 – – –
Hunt & Reffert 2023 8.31 2.63 1.89 650 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2946 98.5 161.96 -55.87 0.09 -4.24 2.03 50.31 0.21

💡 Note: The % column shows the percentage of members that HSC 2350 shares with each listed object.

Visualization

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