HSC 2765

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0.14 UTI
0.0
CN
0.08
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2765 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age 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 genetic pair P147, along with HSC_2744.

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– 245.77 -49.648 4.185 -9.896 -23.091 -8.492
Hunt & Reffert 2024 245.086 -49.673 4.306 -9.83 -23.593 -4.842
Cavallo et al. 2024 248.006 -47.444 4.32 – – –
Hunt & Reffert 2023 245.086 -49.673 4.306 -9.83 -23.593 -4.842

💡 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– 0.225 0.485 1.0 118 0.350 47 – –
Hunt & Reffert 2024 – – – – – 47(1) – –
Cavallo et al. 2024 0.22 0.75 – 62 0.350 – – –
Hunt & Reffert 2023 0.23 0.22 1.00 173 – – – –

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

Visualization

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