HSC 582

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0.33 UTI
0.28
CN
0.24
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.3 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.24 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 582 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, 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 Low extinction Low mass 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 – 300.143 37.304 0.857 1.011 -0.932 -18.418
Hu & Soubiran 2025 300.209 37.309 – – – –
Hunt & Reffert 2024 300.106 37.411 0.851 1.062 -0.893 -21.509
Cavallo et al. 2024 300.208 37.309 0.847 – – –
Hunt & Reffert 2023 300.106 37.411 0.851 1.062 -0.893 -21.509

💡 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 – – – – -0.230* – – –
Hunt & Reffert 2024 – – – – – 43* – –
Cavallo et al. 2024 1.15 0.50 – 776 0.530 – – –
Hunt & Reffert 2023 1.15 0.42 0.60 561 – – – –

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

Visualization

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