HSC 694

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0.45 UTI
0.27
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.9 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 694 is a poorly populated, very dense object of intermediate 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, old 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.

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– 320.054 44.429 0.232 -4.24 -3.684 -26.724
Hu & Soubiran 2025 320.065 44.432 – – – –
Hunt & Reffert 2024 320.058 44.427 0.243 -4.242 -3.706 -24.994
Cavallo et al. 2024 320.065 44.432 0.25 – – –
Hunt & Reffert 2023 320.058 44.427 0.243 -4.242 -3.706 -24.994

💡 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– 3.645 1.25 0.53 2484 0.010 411 – –
Hu & Soubiran 2025 – – – – -0.190(5) – – –
Hunt & Reffert 2024 – – – – – 411(1) – –
Cavallo et al. 2024 3.36 1.11 – 3388 0.210 – – –
Hunt & Reffert 2023 3.93 1.39 0.53 1581 – – – –

(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 3150 88.9 320.05 44.43 0.23 -4.24 -3.68 -26.72 0.01

💡 Note: The % column shows the percentage of members that HSC 694 shares with each listed object.

Visualization

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