HSC 2722

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0.23 UTI
0.0
CN
0.76
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.76 Dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2722 is a sparse, dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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 Intermediate age

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 – 233.401 -53.02 0.924 -1.286 -1.273 7.3
Hunt & Reffert 2024 233.313 -53.031 0.935 -1.26 -1.311 5.421
Cavallo et al. 2024 233.367 -52.969 0.933 – – –
Hunt & Reffert 2023 233.313 -53.031 0.935 -1.26 -1.311 5.421

💡 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 – – – – – 50* – –
Cavallo et al. 2024 1.09 1.10 – 66 0.200 – – –
Hunt & Reffert 2023 1.01 0.75 0.24 197 – – – –

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

Visualization

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