HSC 224

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0.16 UTI
0.0
CN
0.16
Cdens
0.75
CC3
0.0
Clit
0.88
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.88 Very likely unique

Overview

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HSC 224 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Palma et al. (2025)
Part of multiple system G56, along with CWNU_2666 and OC_0038.

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– 280.244 -11.76 0.558 0.67 -0.71 –
Hunt & Reffert 2024 280.229 -11.804 0.552 0.662 -0.761 -7.752
Cavallo et al. 2024 280.421 -11.514 0.555 – – –
Hunt & Reffert 2023 280.229 -11.804 0.552 0.662 -0.761 -7.752

💡 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– 1.84 2.09 2.46 57 0.480 147 – –
Hunt & Reffert 2024 – – – – – 147(1) – –
Cavallo et al. 2024 2.00 2.21 – 50 0.480 – – –
Hunt & Reffert 2023 1.68 1.97 2.46 64 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2722 12.0 280.56 -11.33 0.56 0.66 -0.82 13.85 0.25

💡 Note: The % column shows the percentage of members that HSC 224 shares with each listed object.

Visualization

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