HSC 220

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0.14 UTI
0.0
CN
0.19
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 220 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by high extinction. It is catalogued as a young 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– 280.738 -12.5 0.579 -0.035 -2.387 23.53
Hunt & Reffert 2024 280.753 -12.487 0.574 -0.02 -2.383 19.011
Hunt & Reffert 2023 280.753 -12.487 0.574 -0.02 -2.383 19.011

💡 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– 1.65 3.18 2.03 56 – 80 – –
Hunt & Reffert 2024 – – – – – 80(1) – –
Hunt & Reffert 2023 1.65 3.18 2.03 56 – – – –

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

Visualization

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