HSC 2590

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0.12 UTI
0.0
CN
0.33
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.33 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2590 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 201.984 -61.874 0.766 -4.894 -3.05 3.725
Hunt & Reffert 2024 201.979 -61.879 0.776 -4.911 -3.068 6.418
Cavallo et al. 2024 202.058 -61.855 0.78 – – –
Hunt & Reffert 2023 201.979 -61.879 0.776 -4.911 -3.068 6.418

💡 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– 1.25 0.795 0.65 163 0.380 107 – –
Hunt & Reffert 2024 – – – – – 107(1) – –
Cavallo et al. 2024 1.25 0.64 – 204 0.380 – – –
Hunt & Reffert 2023 1.25 0.95 0.65 122 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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