HSC 1427

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0.15 UTI
0.0
CN
0.49
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 14.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.49 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1427 is a sparse, loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate 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.

Close Moderate 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 – 81.27 24.459 1.333 -1.821 -5.008 14.315
Hunt & Reffert 2024 81.342 24.342 1.332 -1.851 -4.979 10.259
Cavallo et al. 2024 81.264 24.533 1.332 – – –
Hunt & Reffert 2023 81.342 24.342 1.332 -1.851 -4.979 10.259

💡 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 – – – – – 104* – –
Cavallo et al. 2024 0.72 2.03 – 178 0.270 – – –
Hunt & Reffert 2023 0.70 2.19 0.89 96 – – – –

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

Visualization

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