HSC 1059

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0.13 UTI
0.0
CN
0.15
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1059 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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.

Distant Moderate extinction Near-solar metallicity Young

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 – 30.475 63.632 0.305 -2.086 -0.631 -19.62
Hunt & Reffert 2024 30.473 63.632 0.294 -2.057 -0.63 -19.624
Cavallo et al. 2024 30.499 63.608 0.302 – – –
Hunt & Reffert 2023 30.473 63.632 0.294 -2.057 -0.63 -19.624

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 214* – –
Cavallo et al. 2024 3.37 1.92 – 32 0.190 – – –
Hunt & Reffert 2023 2.88 1.69 0.46 60 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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