HSC 656

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0.17 UTI
0.0
CN
0.37
Cdens
0.5
CC3
0.0
Clit
0.96
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.37 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.96 Unique

Overview

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HSC 656 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Near-solar metallicity Very 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 – 308.716 45.792 0.42 -2.391 -5.529 -17.202
Hunt & Reffert 2024 308.715 45.791 0.413 -2.404 -5.549 -17.195
Cavallo et al. 2024 308.713 45.795 0.413 – – –
Hunt & Reffert 2023 308.715 45.791 0.413 -2.404 -5.549 -17.195

💡 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 – – – – – 131* – –
Cavallo et al. 2024 2.36 1.53 – 15 0.150 – – –
Hunt & Reffert 2023 2.26 1.58 0.28 22 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4149 92.0 308.72 45.79 0.42 -2.39 -5.53 -17.2 0.02
FSR 0260 4.0 308.43 45.63 0.42 -2.22 -4.97 40.48 0.36

💡 Note: The % column shows the percentage of members that HSC 656 shares with each listed object.

Visualization

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