HSC 1228

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0.05 UTI
0.0
CN
0.1
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1228 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 62.488 44.639 1.447 0.029 -3.939 -5.362
Zhang et al. 2024 62.51 44.649 – – – –
Cavallo et al. 2024 62.537 44.49 1.443 – – –
Hunt & Reffert 2023 62.51 44.649 1.441 0.012 -3.979 -1.0

💡 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– 0.67 1.22 0.7 112 0.138 – – –
Zhang et al. 2024 – – – – -0.045(1) – – –
Cavallo et al. 2024 0.68 1.20 – 43 0.320 – – –
Hunt & Reffert 2023 0.66 1.24 0.70 182 – – – –

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

Visualization

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