HSC 543

Click to load Aladin Lite
0.12 UTI
0.0
CN
0.11
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 543 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. 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.

Distant High extinction Massive Near-solar metallicity Very 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 – 300.838 30.435 0.217 -2.81 -5.353 5.689
Hunt & Reffert 2024 300.834 30.423 0.219 -2.792 -5.362 –
Cavallo et al. 2024 300.821 30.456 0.219 – – –
Hunt & Reffert 2023 300.834 30.423 0.219 -2.792 -5.362 –

💡 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 – – – – – 1726* – –
Cavallo et al. 2024 3.50 3.89 – 13 -0.360 – – –
Hunt & Reffert 2023 4.35 4.16 2.66 9 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3542 32.0 300.84 30.42 0.23 -2.86 -5.39 5.69 0.24

💡 Note: The % column shows the percentage of members that HSC 543 shares with each listed object.

Visualization

â„šī¸