HSC 2066

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0.13 UTI
0.0
CN
0.13
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2066 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a moderate 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)
Silver 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– 126.761 -38.887 0.181 -2.759 3.384 -66.473
Hunt & Reffert 2024 126.747 -38.901 0.189 -2.784 3.384 -51.853
Cavallo et al. 2024 126.784 -38.809 0.188 – – –
Hunt & Reffert 2023 126.747 -38.901 0.189 -2.784 3.384 -51.853

💡 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– 5.5 3.31 2.5 39 0.430 419 – –
Hunt & Reffert 2024 – – – – – 419(1) – –
Cavallo et al. 2024 5.89 3.25 – 39 0.430 – – –
Hunt & Reffert 2023 5.11 3.37 2.50 39 – – – –

(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 4041 36.0 126.63 -38.87 0.2 -2.77 3.39 54.37 0.05

💡 Note: The % column shows the percentage of members that HSC 2066 shares with each listed object.

Visualization

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