HSC 663

Click to load Aladin Lite
0.09 UTI
0.0
CN
0.05
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 663 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, 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 High extinction Metal-rich Young

Cavallo et al. (2024)
Silver sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 307.671 46.745 0.234 -3.541 -5.053 -40.981
Hunt & Reffert 2024 307.676 46.743 0.236 -3.518 -5.051 -46.838
Cavallo et al. 2024 307.69 46.747 0.241 – – –
Hunt & Reffert 2023 307.676 46.743 0.236 -3.518 -5.051 -46.838

💡 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 – – – – – 148* – –
Cavallo et al. 2024 4.35 3.50 – 22 0.770 – – –
Hunt & Reffert 2023 3.95 4.08 2.29 27 – – – –

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

Visualization

â„šī¸