HSC 946

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0.07 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 946 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 2.573 65.346 0.138 -2.057 -0.121 -20.602
Hunt & Reffert 2024 2.428 65.341 0.149 -2.052 -0.12 -20.602
Hunt & Reffert 2023 2.428 65.341 0.149 -2.052 -0.12 -20.602

💡 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– 6.17 4.08 2.22 154 – 1196 – –
Hunt & Reffert 2024 – – – – – 1196(1) – –
Hunt & Reffert 2023 6.17 4.08 2.22 154 – – – –

(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 4015 88.0 2.58 65.35 0.15 -2.05 -0.12 -20.6 0.01

💡 Note: The % column shows the percentage of members that HSC 946 shares with each listed object.

Visualization

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