HSC 1601

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0.17 UTI
0.0
CN
0.11
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1601 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively 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.

Relatively 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 – 89.832 5.463 0.64 0.003 2.785 35.319
Hu & Soubiran 2025 89.783 5.52 – – – –
Hunt & Reffert 2024 89.832 5.459 0.633 -0.007 2.763 35.373
Cavallo et al. 2024 89.783 5.52 0.636 – – –
Hunt & Reffert 2023 89.832 5.459 0.633 -0.007 2.763 35.373

💡 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 – – – – -0.280* – – –
Hunt & Reffert 2024 – – – – – 82* – –
Cavallo et al. 2024 1.82 2.10 – 550 -0.030 – – –
Hunt & Reffert 2023 1.50 1.86 1.01 184 – – – –

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

Visualization

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