HSC 2353

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0.16 UTI
0.0
CN
0.31
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.31 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2353 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low 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 optical pair P465, along with Theia_1982.

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– 157.738 -60.257 0.359 -5.96 2.338 –
Hunt & Reffert 2024 157.762 -60.259 0.359 -5.947 2.335 –
Cavallo et al. 2024 157.743 -60.257 0.36 – – –
Hunt & Reffert 2023 157.762 -60.259 0.359 -5.947 2.335 –

💡 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– 2.535 0.98 0.46 36 -0.030 101 – –
Hunt & Reffert 2024 – – – – – 101(1) – –
Cavallo et al. 2024 2.41 0.95 – 31 -0.030 – – –
Hunt & Reffert 2023 2.66 1.01 0.46 40 – – – –

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

Visualization

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