HSC 1355

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0.05 UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1355 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, well below the mid-plane. It is catalogued as a near-solar metallicity cluster (see Parameters). It was recently reported in the literature.

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– 64.818 22.7 0.12 0.507 -0.767 –
Zhang et al. 2024 64.829 22.695 – – – –
Hunt & Reffert 2024 64.829 22.695 0.178 0.559 -0.787 -3.513

💡 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– – – – – -0.470 71 – –
Zhang et al. 2024 – – – – -0.470(1) – – –
Hunt & Reffert 2024 – – – – – 71(1) – –

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

Visualization

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