HSC 1027

Click to load Aladin Lite
0.15 UTI
0.0
CN
0.52
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.52 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1027 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as an 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.

Palma et al. (2025)
Classified as optical pair P405, along with Theia_4940.

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

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 28.683 71.07 0.978 -0.048 -1.786 -14.364
Hunt & Reffert 2023 28.793 71.084 0.966 -0.043 -1.768 -14.37

💡 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– 0.98 0.72 0.49 117 – – – –
Hunt & Reffert 2023 0.98 0.72 0.49 117 – – – –

Visualization

â„šī¸