HSC 2714

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0.17 UTI
0.0
CN
0.35
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 15.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.35 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2714 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a metal-poor, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 Metal-poor Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 245.628 -63.022 1.351 -6.179 -9.276 -7.496
Hu & Soubiran 2025 245.572 -63.058 – – – –
Cavallo et al. 2024 245.572 -63.058 1.359 – – –
Hunt & Reffert 2023 245.707 -63.031 1.358 -6.229 -9.339 -5.925

💡 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
Hu & Soubiran 2025 – – – – -0.210* – – –
Cavallo et al. 2024 0.71 0.66 – 741 -0.950 – – –
Hunt & Reffert 2023 0.68 0.13 0.38 679 – – – –

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

Visualization

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