HSC 2653

Click to load Aladin Lite
0.09 UTI
0.0
CN
0.07
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2653 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low 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.

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– 222.521 -68.452 2.544 -11.033 -5.304 -9.236
Cavallo et al. 2024 222.61 -68.556 2.581 – – –
Hunt & Reffert 2023 225.329 -68.005 2.583 -10.891 -5.291 -7.419

💡 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– 0.4 0.515 0.26 28 -0.010 – – –
Cavallo et al. 2024 0.43 0.85 – 12 -0.010 – – –
Hunt & Reffert 2023 0.37 0.18 0.26 44 – – – –

Visualization

â„šī¸