HSC 2564

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0.50 UTI
0.26
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.26 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 2564 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 198.084 -62.898 0.397 -5.141 -2.042 –
Hu & Soubiran 2025 198.029 -62.888 – – – –
Hunt & Reffert 2024 198.074 -62.9 0.391 -5.159 -2.059 –
Cavallo et al. 2024 198.029 -62.888 0.393 – – –
Hunt & Reffert 2023 198.074 -62.9 0.391 -5.159 -2.059 –

💡 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 – – – – -0.100* – – –
Hunt & Reffert 2024 – – – – – 301* – –
Cavallo et al. 2024 2.09 3.00 – 891 0.130 – – –
Hunt & Reffert 2023 2.29 2.96 2.02 348 – – – –

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

Visualization

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