HSC 1625

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0.40 UTI
0.27
CN
1.0
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.5 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1625 is a poorly populated, very dense object of low 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 (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– 98.306 5.373 0.211 0.013 0.868 80.412
Hu & Soubiran 2025 98.33 5.377 – – – –
Hunt & Reffert 2024 98.309 5.375 0.193 0.05 0.801 80.417
Cavallo et al. 2024 98.33 5.377 0.198 – – –
Hunt & Reffert 2023 98.309 5.375 0.193 0.05 0.801 80.417

💡 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– 4.585 2.78 1.58 604 -0.395 382 – –
Hu & Soubiran 2025 – – – – -0.410(5) – – –
Hunt & Reffert 2024 – – – – – 382(1) – –
Cavallo et al. 2024 4.97 2.91 – 646 -0.380 – – –
Hunt & Reffert 2023 4.20 2.65 1.58 562 – – – –

(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 3607 100.0 98.31 5.37 0.2 0.02 0.87 80.41 0.18

💡 Note: The % column shows the percentage of members that HSC 1625 shares with each listed object.

Visualization

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