HSC 1833

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0.14 UTI
0.0
CN
0.07
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1833 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, above 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 P136, along with UPK_468.

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 99999– 118.805 -12.409 1.033 -5.359 3.064 38.42
Cavallo et al. 2024 118.685 -12.309 1.045 – – –
Hunt & Reffert 2023 118.92 -12.552 1.023 -5.336 3.056 36.795

💡 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– 0.955 0.2 0.41 62 -0.030 – – –
Cavallo et al. 2024 1.00 0.26 – 26 -0.030 – – –
Hunt & Reffert 2023 0.91 0.14 0.41 99 – – – –

Visualization

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