HSC 920

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0.09 UTI
0.0
CN
0.18
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 920 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 356.28 62.756 0.504 -2.201 -1.958 –
Hunt & Reffert 2024 356.34 62.793 0.512 -2.182 -1.968 –
Cavallo et al. 2024 356.26 62.769 0.511 – – –
Hunt & Reffert 2023 356.34 62.793 0.512 -2.182 -1.968 –

💡 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– 1.83 2.325 1.69 182 0.580 97 – –
Hunt & Reffert 2024 – – – – – 97(1) – –
Cavallo et al. 2024 1.79 2.14 – 257 0.580 – – –
Hunt & Reffert 2023 1.87 2.51 1.69 106 – – – –

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

Visualization

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