HSC 1060

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0.17 UTI
0.0
CN
0.06
Cdens
0.75
CC3
0.06
Clit
0.88
Cdup
Core radius and density 2.3 [pc], 0.3 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.06 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

â„šī¸
HSC 1060 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-rich, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a 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=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Liu et al. (2025)
Classified as primordial binary cluster 33 along with Berkeley_7.

Palma et al. (2025)
Classified as genetic pair P188, along with Berkeley_7.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 29.519 61.913 0.341 -1.027 -0.391 -15.47
Hunt & Reffert 2024 29.496 61.938 0.341 -1.024 -0.39 -15.498
Cavallo et al. 2024 29.552 61.856 0.344 – – –
Hunt & Reffert 2023 29.496 61.938 0.341 -1.024 -0.39 -15.498

💡 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– 2.905 1.645 1.79 34 1.040 319 – –
Liu et al. 2025 5.01 0.60 – 44 – – – –
Hunt & Reffert 2024 2.65 1.86 1.79 24 – 319(1) – –
Cavallo et al. 2024 3.16 1.43 – 72 1.040 – – –
Hunt & Reffert 2023 2.65 1.86 1.79 24 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2006 12.0 28.92 61.99 0.33 -1.07 -0.31 – 0.08
CWWDL 8417 4.0 28.64 61.78 0.35 -1.12 -0.39 – 0.1
CWWDL 8449 4.0 29.76 62.03 0.34 -1.01 -0.22 – 0.05

💡 Note: The % column shows the percentage of members that HSC 1060 shares with each listed object.

Visualization

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