HSC 823

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0.11 UTI
0.0
CN
0.16
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 17.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 823 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Moderate extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 333.343 61.419 0.991 -3.568 -3.647 -20.416
Hu & Soubiran 2025 333.359 61.496 – – – –
Cavallo et al. 2024 333.359 61.496 0.992 – – –
Hunt & Reffert 2023 333.435 61.41 0.991 -3.539 -3.65 -20.419

💡 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 – – – – -0.010* – – –
Cavallo et al. 2024 0.90 1.55 – 1738 -0.380 – – –
Hunt & Reffert 2023 0.97 1.82 1.53 402 – – – –

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

Visualization

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