HSC 522

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0.27 UTI
0.25
CN
0.25
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 522 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low 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 Low 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 – 297.212 29.228 0.677 0.678 -1.227 -19.933
Hu & Soubiran 2025 297.215 29.152 – – – –
Hunt & Reffert 2024 297.359 29.303 0.676 0.697 -1.222 -19.967
Cavallo et al. 2024 297.215 29.152 0.677 – – –
Hunt & Reffert 2023 297.359 29.303 0.676 0.697 -1.222 -19.967

💡 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 – – – – -0.060* – – –
Hunt & Reffert 2024 – – – – – 68* – –
Cavallo et al. 2024 1.45 0.20 – 1148 0.260 – – –
Hunt & Reffert 2023 1.40 0.82 0.90 202 – – – –

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

Visualization

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