HSC 1366

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0.09 UTI
0.0
CN
0.19
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.19 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 1366 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, 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 Metal-rich 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 – 86.584 35.194 0.35 1.165 -2.422 13.575
Hunt & Reffert 2024 86.625 35.154 0.336 1.17 -2.425 13.633
Cavallo et al. 2024 86.574 35.175 0.336 – – –
Hunt & Reffert 2023 86.625 35.154 0.336 1.17 -2.425 13.633

💡 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 – – – – – 328* – –
Cavallo et al. 2024 2.96 2.58 – 257 0.670 – – –
Hunt & Reffert 2023 2.78 2.30 1.85 389 – – – –

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

Visualization

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