HSC 1539

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0.18 UTI
0.34
CN
0.14
Cdens
0.25
CC3
0.1
Clit
1.0
Cdup
Core radius and density 2.0 [pc], 0.7 [pc-2]
  • CN 0.34 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.25 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1539 is a poorly populated, 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 near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (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 open cluster. CMD class: 0.49 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.49 (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– 90.729 14.594 1.15 -1.599 -1.528 5.228
Yang et al. 2025 90.691 14.594 – – – –
Zhang et al. 2024 90.691 14.594 – – – –
Hunt & Reffert 2024 90.691 14.594 1.145 -1.577 -1.491 14.879
Cavallo et al. 2024 90.674 14.596 1.145 – – –
Hunt & Reffert 2023 90.691 14.594 1.145 -1.577 -1.491 14.879

💡 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– 0.83 0.37 0.86 36 -0.185 95 – –
Yang et al. 2025 – – – 36 -0.190(3) – – –
Zhang et al. 2024 – – – – -0.185(1) – – –
Hunt & Reffert 2024 0.83 0.37 0.86 36 – 95(1) – –
Cavallo et al. 2024 1.01 0.53 – 19 0.150 – – –
Hunt & Reffert 2023 0.83 0.37 0.86 36 – – – –

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

Visualization

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