HSC 1666

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0.04 UTI
0.0
CN
0.08
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 40.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1666 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low 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 Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

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

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 105.184 1.672 1.607 -1.74 -1.124 5.518
Zhang et al. 2024 104.752 3.317 – – – –
Cavallo et al. 2024 105.349 0.656 1.596 – – –
Hunt & Reffert 2023 104.752 3.317 1.604 -1.668 -1.144 7.669

💡 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
Zhang et al. 2024 – – – – -0.121* – – –
Cavallo et al. 2024 0.63 0.24 – 107 -0.110 – – –
Hunt & Reffert 2023 0.60 0.09 0.45 249 – – – –

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

Visualization

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