HSC 515

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0.11 UTI
0.0
CN
0.18
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Core radius and density 1.8 [pc], 0.9 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 515 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, 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)
Silver sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.85 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.85 (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– 300.611 26.683 0.546 -3.342 -3.737 31.996
Cavallo et al. 2024 300.662 26.695 0.576 – – –
Hunt & Reffert 2023 300.621 26.692 0.576 -3.308 -3.733 33.671

💡 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– 2.195 2.87 0.62 966 -0.930 – – –
Cavallo et al. 2024 2.56 3.29 – 603 -0.930 – – –
Hunt & Reffert 2023 1.83 2.45 0.62 1330 – – – –

Visualization

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