HSC 1350

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0.23 UTI
0.0
CN
0.15
Cdens
0.38
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.38 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1350 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (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.

Liu et al. (2025)
Classified as primordial binary cluster 81 along with CWNU_525.

Palma et al. (2025)
Part of multiple system G113, along with NGC_1912, CWNU_525 and Teutsch_89.

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– 83.798 36.003 0.879 -0.332 -3.091 -0.841
Zhang et al. 2024 83.849 35.993 – – – –
Hunt & Reffert 2024 83.849 35.993 0.873 -0.346 -3.104 -12.856
Cavallo et al. 2024 83.462 36.023 0.873 – – –
Hunt & Reffert 2023 83.849 35.993 0.873 -0.346 -3.104 -12.856

💡 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– 1.21 0.87 0.55 40 0.102 49 – –
Liu et al. 2025 1.79 0.37 – 26 – – – –
Zhang et al. 2024 – – – – -0.176(1) – – –
Hunt & Reffert 2024 – – – – – 49(1) – –
Cavallo et al. 2024 1.21 0.89 – 40 0.380 – – –
Hunt & Reffert 2023 1.08 0.87 0.55 52 – – – –

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

Visualization

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