HSC 1927

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0.43 UTI
0.26
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.7 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1927 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 low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the absorption 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– 111.801 -27.172 0.231 -1.694 3.644 82.884
Hu & Soubiran 2025 111.826 -27.17 – – – –
Hunt & Reffert 2024 111.803 -27.179 0.233 -1.689 3.585 82.845
Cavallo et al. 2024 111.826 -27.17 0.225 – – –
Hunt & Reffert 2023 111.803 -27.179 0.233 -1.689 3.585 82.845

💡 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– 4.22 0.88 0.81 2285 -0.360 218 – –
Hu & Soubiran 2025 – – – – -0.400(5) – – –
Hunt & Reffert 2024 – – – – – 218(1) – –
Cavallo et al. 2024 4.55 1.49 – 1349 -0.320 – – –
Hunt & Reffert 2023 3.89 0.27 0.81 3221 – – – –

(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 2986 92.3 111.8 -27.18 0.24 -1.69 3.64 82.88 0.03

💡 Note: The % column shows the percentage of members that HSC 1927 shares with each listed object.

Visualization

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