HSC 2584

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0.36 UTI
0.38
CN
0.19
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.8 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.19 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2584 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 moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 – 202.237 -64.78 0.362 -9.041 -1.921 -45.16
Hu & Soubiran 2025 202.163 -64.773 – – – –
Hunt & Reffert 2024 202.146 -64.777 0.365 -9.033 -1.919 -46.307
Cavallo et al. 2024 202.163 -64.773 0.365 – – –
Hunt & Reffert 2023 202.146 -64.777 0.365 -9.033 -1.919 -46.307

💡 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 – – – – -0.350* – – –
Hunt & Reffert 2024 – – – – – 200* – –
Cavallo et al. 2024 2.25 1.32 – 1096 0.070 – – –
Hunt & Reffert 2023 2.54 1.54 2.11 244 – – – –

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

Visualization

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