HSC 826

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0.37 UTI
0.29
CN
0.31
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.31 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 826 is a poorly populated, 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 – 341.422 56.328 0.451 -1.9 -2.784 -44.559
Hu & Soubiran 2025 341.372 56.357 – – – –
Hunt & Reffert 2024 341.429 56.33 0.45 -1.888 -2.785 -33.727
Cavallo et al. 2024 341.372 56.357 0.452 – – –
Hunt & Reffert 2023 341.429 56.33 0.45 -1.888 -2.785 -33.727

💡 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 – – – – -0.130* – – –
Hunt & Reffert 2024 – – – – – 251* – –
Cavallo et al. 2024 2.27 1.64 – 589 0.230 – – –
Hunt & Reffert 2023 2.10 1.28 0.37 1002 – – – –

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

Visualization

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