HSC 758

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0.19 UTI
0.25
CN
0.22
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 758 is a poorly populated, 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 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.

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– 325.485 54.736 6.974 20.512 5.204 -20.753
Cavallo et al. 2024 325.149 54.488 6.978 – – –
Hunt & Reffert 2023 323.983 55.117 6.978 20.356 5.115 -26.912

💡 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– 0.145 0.56 0.71 65 0.100 – – –
Cavallo et al. 2024 0.15 0.57 – 78 0.100 – – –
Hunt & Reffert 2023 0.14 0.55 0.71 52 – – – –

Visualization

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