HSC 1761

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0.21 UTI
0.44
CN
0.23
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Core radius and density 1.3 [pc], 1.1 [pc-2]
  • CN 0.44 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1761 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 105.672 -10.634 1.558 -4.634 -1.973 21.28
Cavallo et al. 2024 105.676 -10.577 1.572 – – –
Hunt & Reffert 2023 105.608 -10.619 1.566 -4.514 -1.984 19.901

💡 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– 0.615 0.185 0.48 191 0.040 – – –
Cavallo et al. 2024 0.63 0.25 – 200 0.040 – – –
Hunt & Reffert 2023 0.60 0.12 0.48 182 – – – –

Visualization

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