HSC 533

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0.24 UTI
0.25
CN
0.32
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 17.1 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.32 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 533 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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.

Close Low extinction Near-solar metallicity Young

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 – 298.682 30.06 1.265 2.068 0.974 -12.03
Hunt & Reffert 2024 298.666 30.077 1.242 2.148 0.898 -12.406
Cavallo et al. 2024 298.647 30.096 1.244 – – –
Hunt & Reffert 2023 298.666 30.077 1.242 2.148 0.898 -12.406

💡 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 – – – – – 73* – –
Cavallo et al. 2024 0.85 1.32 – 26 -0.090 – – –
Hunt & Reffert 2023 0.75 0.61 0.88 61 – – – –

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

Visualization

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