HSC 818

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0.50 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 818 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant 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 – 337.024 58.167 0.256 -5.571 -3.397 -65.414
Hu & Soubiran 2025 337.054 58.183 – – – –
Hunt & Reffert 2024 337.019 58.165 0.247 -5.56 -3.389 -65.412
Cavallo et al. 2024 337.054 58.183 0.244 – – –
Hunt & Reffert 2023 337.019 58.165 0.247 -5.56 -3.389 -65.412

💡 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 – – – – – 281* – –
Cavallo et al. 2024 2.92 1.85 – 794 -0.050 – – –
Hunt & Reffert 2023 3.65 2.40 1.20 199 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3221 100.0 337.01 58.17 0.25 -5.52 -3.4 -65.41 0.19

💡 Note: The % column shows the percentage of members that HSC 818 shares with each listed object.

Visualization

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