HSC 118

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0.20 UTI
0.34
CN
0.29
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 118 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, 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)
Part of multiple system G54, along with vdBergh_113, CWNU_482 and CWNU_2597.

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 272.604 -22.354 0.67 1.179 -3.154 -24.56
Hunt & Reffert 2024 272.658 -22.47 0.683 1.209 -3.179 -23.49
Cavallo et al. 2024 272.582 -22.384 0.683 – – –
Hunt & Reffert 2023 272.658 -22.47 0.683 1.209 -3.179 -23.49

💡 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– 1.24 2.315 2.62 33 -0.840 191 – –
Hunt & Reffert 2024 – – – – – 191(1) – –
Cavallo et al. 2024 1.06 2.80 – 46 -0.840 – – –
Hunt & Reffert 2023 1.42 1.83 2.62 20 – – – –

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

Visualization

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