HSC 2533

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0.16 UTI
0.0
CN
0.44
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.44 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2533 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively 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.

Relatively 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 – 191.788 -65.487 0.901 -6.872 -1.316 -6.253
Hunt & Reffert 2024 191.845 -65.528 0.905 -6.901 -1.316 -10.619
Cavallo et al. 2024 191.752 -65.503 0.905 – – –
Hunt & Reffert 2023 191.845 -65.528 0.905 -6.901 -1.316 -10.619

💡 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 – – – – – 93* – –
Cavallo et al. 2024 1.22 0.73 – 58 0.380 – – –
Hunt & Reffert 2023 1.06 0.82 0.52 79 – – – –

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

Visualization

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