HSC 488

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0.15 UTI
0.0
CN
0.38
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.38 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 488 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age 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– 297.818 23.131 0.224 -0.791 -4.109 6.849
Hunt & Reffert 2024 297.822 23.137 0.212 -0.803 -4.137 9.355
Hunt & Reffert 2023 297.822 23.137 0.212 -0.803 -4.137 9.355

💡 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– 4.38 3.37 1.65 316 – 215 – –
Hunt & Reffert 2024 – – – – – 215(1) – –
Hunt & Reffert 2023 4.38 3.37 1.65 316 – – – –

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

Visualization

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