HSC 1731

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0.49 UTI
0.56
CN
0.39
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.56 Moderately populated
  • Cdens 0.39 Loose
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1731 is a moderately populated, loose object of very high C3 quality. Its parallax locates it at a very large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~10.20 kpc) differs significantly from the median photometric distance (~6.85 kpc).

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

Very distant Moderate extinction Metal-poor 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 – 98.666 -8.859 0.098 0.174 0.443 69.459
Hu & Soubiran 2025 98.663 -8.858 – – – –
Hunt & Reffert 2024 98.654 -8.865 0.085 0.163 0.458 69.479
Cavallo et al. 2024 98.663 -8.858 0.09 – – –
Hunt & Reffert 2023 98.654 -8.865 0.085 0.163 0.458 69.479

💡 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 – – – – -0.310* – – –
Hunt & Reffert 2024 – – – – – 978* – –
Cavallo et al. 2024 5.08 1.87 – 1175 -0.870 – – –
Hunt & Reffert 2023 8.62 1.60 0.78 643 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2972 98.4 98.66 -8.86 0.11 0.16 0.45 69.46 0.07

💡 Note: The % column shows the percentage of members that HSC 1731 shares with each listed object.

Visualization

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