HSC 1166

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0.09 UTI
0.0
CN
0.1
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 24.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1166 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, above 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)
Wood 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 – 68.318 62.638 1.024 3.03 -8.435 -18.81
Cavallo et al. 2024 68.241 62.734 1.03 – – –
Hunt & Reffert 2023 68.322 62.769 1.039 3.138 -8.451 -18.693

💡 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
Cavallo et al. 2024 1.43 1.90 – 110 0.070 – – –
Hunt & Reffert 2023 0.93 2.13 1.73 745 – – – –

Visualization

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