HSC 113

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0.10 UTI
0.0
CN
0.01
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 113 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old 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.

Very distant Moderate extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 279.765 -26.545 0.117 -3.97 -4.644 -44.246
Hu & Soubiran 2025 279.75 -26.543 – – – –
Cavallo et al. 2024 279.75 -26.543 0.122 – – –
Hunt & Reffert 2023 279.771 -26.557 0.122 -3.924 -4.684 -6.954

💡 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] Bfr BSS
Hu & Soubiran 2025 – – – – -0.300* – – –
Cavallo et al. 2024 7.28 1.18 – 7079 -0.390 – – –
Hunt & Reffert 2023 6.97 1.69 1.35 1574 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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