HSC 572

Click to load Aladin Lite
0.17 UTI
0.25
CN
0.22
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 572 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It was recently reported in the literature.

Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

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– 290.939 40.636 3.183 -3.887 3.06 -24.653
Zhang et al. 2024 290.682 40.622 – – – –
Cavallo et al. 2024 290.459 39.919 3.121 – – –
Hunt & Reffert 2023 290.682 40.622 3.127 -3.919 2.878 -23.896

💡 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– 0.32 0.24 0.35 76 0.038 – – –
Zhang et al. 2024 – – – – 0.036(1) – – –
Cavallo et al. 2024 0.33 0.46 – 47 0.040 – – –
Hunt & Reffert 2023 0.31 0.02 0.35 104 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 569 28.0 289.3 40.62 3.44 -4.7 3.3 -22.33 0.16

💡 Note: The % column shows the percentage of members that HSC 572 shares with each listed object.

Visualization

â„šī¸