HSC 588

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0.13 UTI
0.0
CN
0.17
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.17 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 588 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P611, along with Dolidze_3.

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– 302.753 37.318 0.499 -2.785 -5.704 –
Hunt & Reffert 2024 302.729 37.293 0.498 -2.798 -5.681 –
Cavallo et al. 2024 302.73 37.33 0.499 – – –
Hunt & Reffert 2023 302.729 37.293 0.498 -2.798 -5.681 –

💡 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– 1.885 1.405 0.86 20 0.440 247 – –
Hunt & Reffert 2024 – – – – – 247(1) – –
Cavallo et al. 2024 1.85 1.23 – 33 0.440 – – –
Hunt & Reffert 2023 1.92 1.58 0.86 7 – – – –

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

Visualization

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