HSC 2280

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0.14 UTI
0.0
CN
0.21
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Core radius and density 1.2 [pc], 1.0 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2280 is a sparse, very loose object of intermediate 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: 0.95 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.95 (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– 148.943 -56.226 1.741 -18.525 11.19 3.983
Cavallo et al. 2024 149.117 -56.278 1.759 – – –
Hunt & Reffert 2023 148.78 -56.261 1.764 -18.591 11.229 4.488

💡 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– 0.555 0.41 0.48 160 0.180 – – –
Cavallo et al. 2024 0.57 0.56 – 182 0.180 – – –
Hunt & Reffert 2023 0.54 0.26 0.48 139 – – – –

Visualization

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