HSC 2364

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0.33 UTI
0.29
CN
0.13
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.4 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.13 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2364 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 158.106 -61.32 0.41 -4.891 2.027 26.837
Hu & Soubiran 2025 158.09 -61.31 – – – –
Hunt & Reffert 2024 158.055 -61.337 0.407 -4.898 2.029 28.215
Cavallo et al. 2024 158.09 -61.31 0.411 – – –
Hunt & Reffert 2023 158.055 -61.337 0.407 -4.898 2.029 28.215

💡 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 – – – – -0.250* – – –
Hunt & Reffert 2024 – – – – – 112* – –
Cavallo et al. 2024 2.00 1.12 – 1072 0.020 – – –
Hunt & Reffert 2023 2.27 0.67 0.42 902 – – – –

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

Visualization

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