HSC 786

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0.10 UTI
0.0
CN
0.14
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 786 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate 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– 322.483 61.589 1.037 -4.532 -4.677 -14.357
Cavallo et al. 2024 322.535 61.57 1.032 – – –
Hunt & Reffert 2023 322.463 61.579 1.025 -4.512 -4.631 -9.651

💡 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– 1.01 1.245 0.63 74 0.440 – – –
Cavallo et al. 2024 1.09 1.29 – 58 0.440 – – –
Hunt & Reffert 2023 0.93 1.20 0.63 90 – – – –

Visualization

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