HSC 546

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0.11 UTI
0.0
CN
0.16
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 546 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a metal-poor, 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.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 302.178 29.839 0.215 -2.347 -5.078 -8.572
Hunt & Reffert 2024 302.209 29.838 0.21 -2.354 -5.087 -10.277
Cavallo et al. 2024 302.159 29.855 0.211 – – –
Hunt & Reffert 2023 302.209 29.838 0.21 -2.354 -5.087 -10.277

💡 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– 4.875 4.65 1.47 318 -0.530 640 – –
Hunt & Reffert 2024 – – – – – 640(1) – –
Cavallo et al. 2024 5.73 4.78 – 347 -0.530 – – –
Hunt & Reffert 2023 4.02 4.52 1.47 290 – – – –

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

Visualization

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