HSC 1476

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0.17 UTI
0.35
CN
0.12
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 6.3 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.12 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1476 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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.

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 Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 89.945 23.659 0.239 0.476 -0.299 16.124
Hunt & Reffert 2024 89.965 23.646 0.238 0.439 -0.319 –
Cavallo et al. 2024 89.805 23.74 0.232 – – –
Hunt & Reffert 2023 89.965 23.646 0.238 0.439 -0.319 –

💡 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 – – – – – 347* – –
Cavallo et al. 2024 4.19 2.68 – 51 0.410 – – –
Hunt & Reffert 2023 3.74 2.78 2.51 28 – – – –

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

Visualization

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