HSC 2136

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0.10 UTI
0.0
CN
0.17
Cdens
0.38
CC3
0.0
Clit
0.96
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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HSC 2136 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) 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 a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 135.41 -43.237 1.214 -9.513 5.691 15.493
Hu & Soubiran 2025 135.568 -43.242 – – – –
Cavallo et al. 2024 135.568 -43.242 1.216 – – –
Hunt & Reffert 2023 135.393 -43.303 1.213 -9.55 5.715 12.162

💡 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– 0.82 0.235 0.29 3814 0.420 – – –
Cavallo et al. 2024 0.86 0.38 – 2344 0.420 – – –
Hunt & Reffert 2023 0.78 0.09 0.29 5284 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 182 4.0 135.92 -43.94 1.05 -8.75 5.78 28.67 0.33

💡 Note: The % column shows the percentage of members that HSC 2136 shares with each listed object.

Visualization

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