HSC 1858

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0.27 UTI
0.3
CN
0.28
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.28 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1858 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Gold 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– 112.901 -19.399 0.351 -2.33 3.441 –
Hunt & Reffert 2024 112.902 -19.422 0.348 -2.33 3.432 –
Cavallo et al. 2024 112.921 -19.403 0.349 – – –
Hunt & Reffert 2023 112.902 -19.422 0.348 -2.33 3.432 –

💡 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– 2.72 1.515 0.75 132 -0.010 303 – –
Hunt & Reffert 2024 – – – – – 303(1) – –
Cavallo et al. 2024 2.82 1.52 – 174 -0.010 – – –
Hunt & Reffert 2023 2.62 1.51 0.75 91 – – – –

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

Visualization

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