HSC 1822

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0.27 UTI
0.0
CN
0.11
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1822 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, old cluster (see Parameters). It was recently reported in the literature.
Distant Moderate extinction Metal-poor Old

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 – 110.727 -16.086 0.195 -0.402 1.273 79.529
Hu & Soubiran 2025 110.731 -16.111 – – – –
Hunt & Reffert 2024 110.703 -16.086 0.184 -0.399 1.292 78.156
Cavallo et al. 2024 110.731 -16.111 0.186 – – –
Hunt & Reffert 2023 110.703 -16.086 0.184 -0.399 1.292 78.156

💡 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 – – – – -0.450* – – –
Hunt & Reffert 2024 – – – – – 697* – –
Cavallo et al. 2024 4.74 3.03 – 4571 -0.750 – – –
Hunt & Reffert 2023 4.63 2.65 1.00 5297 – – – –

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

Visualization

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