HSC 457

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0.14 UTI
0.0
CN
0.21
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.21 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 457 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very 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 High extinction Near-solar metallicity Very 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 – 294.795 20.143 0.258 -2.546 -6.12 101.945
Hunt & Reffert 2024 294.817 20.173 0.262 -2.562 -6.145 101.899
Cavallo et al. 2024 294.778 20.124 0.261 – – –
Hunt & Reffert 2023 294.817 20.173 0.262 -2.562 -6.145 101.899

💡 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 – – – – – 752* – –
Cavallo et al. 2024 4.17 3.57 – 8 -0.200 – – –
Hunt & Reffert 2023 3.46 3.67 2.41 13 – – – –

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

Visualization

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