HSC 665

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0.43 UTI
0.39
CN
1.0
Cdens
0.38
CC3
0.25
Clit
0.95
Cdup
Radius (P>50% members) 1.5 [arcmin]
  • CN 0.39 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.95 Unique

Overview

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HSC 665 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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 is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close 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 – 310.597 45.495 0.31 -3.348 -5.137 –
Hu & Soubiran 2025 310.597 45.492 – – – –
Hunt & Reffert 2024 310.596 45.494 0.305 -3.337 -5.119 –
Cavallo et al. 2024 310.597 45.492 0.306 – – –
Hunt & Reffert 2023 310.596 45.494 0.305 -3.337 -5.119 –

💡 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 – – – – -0.260* – – –
Hunt & Reffert 2024 – – – – – 451* – –
Cavallo et al. 2024 2.70 1.98 – 617 0.310 – – –
Hunt & Reffert 2023 2.91 2.69 2.11 211 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3421 92.3 310.6 45.49 0.31 -3.35 -5.14 – 0.02
FoF 1768 5.1 310.69 45.5 0.31 -3.26 -4.78 -38.67 0.04

💡 Note: The % column shows the percentage of members that HSC 665 shares with each listed object.

Visualization

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