HSC 1691

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0.33 UTI
0.4
CN
0.5
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 11.0 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1691 is a poorly populated, moderately dense 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.

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

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 – 106.053 -0.009 0.797 -0.068 -1.829 1.314
Hu & Soubiran 2025 106.039 -0.074 – – – –
Hunt & Reffert 2024 106.077 0.035 0.776 -0.062 -1.805 -2.061
Cavallo et al. 2024 106.039 -0.074 0.781 – – –
Hunt & Reffert 2023 106.077 0.035 0.776 -0.062 -1.805 -2.061

💡 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 – – – – -0.070* – – –
Hunt & Reffert 2024 – – – – – 150* – –
Cavallo et al. 2024 1.32 0.53 – 537 0.450 – – –
Hunt & Reffert 2023 1.18 0.71 0.63 238 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3026 87.5 106.05 -0.06 0.8 -0.07 -1.82 -5.59 0.01

💡 Note: The % column shows the percentage of members that HSC 1691 shares with each listed object.

Visualization

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