HSC 2666

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0.14 UTI
0.0
CN
0.19
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 4.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2666 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate 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)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 226.177 -61.035 0.302 -4.659 -3.73 -29.382
Hunt & Reffert 2024 226.142 -61.058 0.299 -4.671 -3.742 -29.278
Cavallo et al. 2024 226.288 -61.022 0.299 – – –
Hunt & Reffert 2023 226.142 -61.058 0.299 -4.671 -3.742 -29.278

💡 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 – – – – – 157* – –
Cavallo et al. 2024 2.58 1.89 – 191 0.340 – – –
Hunt & Reffert 2023 3.06 2.34 0.65 57 – – – –

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

Visualization

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