HSC 487

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0.10 UTI
0.0
CN
0.13
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Core radius and density 1.6 [pc], 0.6 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 487 is a sparse, 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 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)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (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– 299.699 21.809 1.365 -0.046 -5.625 -13.922
Cavallo et al. 2024 299.442 21.507 1.386 – – –
Hunt & Reffert 2023 299.583 21.832 1.385 -0.015 -5.668 -23.638

💡 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– 0.69 0.88 0.31 162 -0.680 – – –
Cavallo et al. 2024 0.70 1.32 – 85 -0.680 – – –
Hunt & Reffert 2023 0.68 0.44 0.31 238 – – – –

Visualization

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