HSC 1954

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0.17 UTI
0.27
CN
0.06
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 3.0 [pc], 0.3 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.06 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1954 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by low 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.30 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.30 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 117.991 -26.82 0.165 -1.657 2.2 91.228
Hu & Soubiran 2025 118.031 -26.81 – – – –
Hunt & Reffert 2024 117.97 -26.798 0.166 -1.667 2.195 91.721
Cavallo et al. 2024 118.031 -26.81 0.168 – – –
Hunt & Reffert 2023 117.97 -26.798 0.166 -1.667 2.195 91.721

💡 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– 5.45 0.92 2.18 624 -0.085 433 – –
Hu & Soubiran 2025 – – – – -0.210(5) – – –
Hunt & Reffert 2024 5.45 0.92 2.18 623 – 433(1) – –
Cavallo et al. 2024 4.13 0.55 – 1622 0.040 – – –
Hunt & Reffert 2023 5.45 0.92 2.18 624 – – – –

(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 2980 100.0 118.0 -26.82 0.17 -1.66 2.2 91.23 0.02

💡 Note: The % column shows the percentage of members that HSC 1954 shares with each listed object.

Visualization

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