HSC 1065

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0.34 UTI
0.25
CN
0.2
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.0 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.2 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1065 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below 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 age and metallicity parameters (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.

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 99999– 29.601 59.645 0.25 -1.315 -0.231 -50.881
Hu & Soubiran 2025 29.654 59.609 – – – –
Hunt & Reffert 2024 29.599 59.635 0.235 -1.294 -0.256 -82.424
Cavallo et al. 2024 29.654 59.609 0.239 – – –
Hunt & Reffert 2023 29.599 59.635 0.235 -1.294 -0.256 -82.424

💡 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] Bfrac BSS
UCC 99999– 3.51 1.52 1.91 328 0.250 329 – –
Hu & Soubiran 2025 – – – – -0.170(5) – – –
Hunt & Reffert 2024 – – – – – 329(1) – –
Cavallo et al. 2024 3.50 1.27 – 562 0.670 – – –
Hunt & Reffert 2023 3.52 1.77 1.91 95 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3454 84.0 29.6 59.64 0.25 -1.31 -0.22 -50.88 0.04

💡 Note: The % column shows the percentage of members that HSC 1065 shares with each listed object.

Visualization

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