HSC 1085

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0.23 UTI
0.0
CN
0.77
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.77 Dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1085 is a sparse, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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.

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– 34.596 60.671 0.424 -0.998 -0.321 -15.823
Hunt & Reffert 2024 34.597 60.666 0.419 -1.01 -0.268 -15.835
Cavallo et al. 2024 35.134 60.727 0.422 – – –
Hunt & Reffert 2023 34.597 60.666 0.419 -1.01 -0.268 -15.835

💡 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– 2.2 3.395 2.59 44 -0.020 127 – –
Hunt & Reffert 2024 – – – – – 127(1) – –
Cavallo et al. 2024 2.22 3.42 – 55 -0.020 – – –
Hunt & Reffert 2023 2.18 3.37 2.59 32 – – – –

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

Visualization

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