HSC 1859

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0.18 UTI
0.25
CN
0.16
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1859 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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.

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 110.229 -20.781 0.344 -2.288 3.188 –
Hunt & Reffert 2024 110.237 -20.775 0.337 -2.321 3.188 –
Cavallo et al. 2024 110.249 -20.749 0.337 – – –
Hunt & Reffert 2023 110.237 -20.775 0.337 -2.321 3.188 –

💡 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– 2.84 1.305 0.43 32 -0.150 152 – –
Hunt & Reffert 2024 – – – – – 152(1) – –
Cavallo et al. 2024 3.01 1.23 – 12 -0.150 – – –
Hunt & Reffert 2023 2.67 1.38 0.43 53 – – – –

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

Visualization

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