HSC 1531

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0.19 UTI
0.0
CN
0.55
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.55 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1531 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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.

Palma et al. (2025)
Classified as optical pair P292, along with CWNU_1111.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 87.205 13.889 3.615 5.08 -13.123 22.424
Zhang et al. 2024 87.328 13.836 – – – –
Cavallo et al. 2024 87.273 14.41 3.612 – – –
Hunt & Reffert 2023 87.328 13.836 3.616 5.181 -13.155 15.577

💡 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– 0.27 0.4 0.59 56 0.074 – – –
Zhang et al. 2024 – – – – 0.099(1) – – –
Cavallo et al. 2024 0.27 0.64 – 31 0.050 – – –
Hunt & Reffert 2023 0.27 0.16 0.59 81 – – – –

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

Visualization

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