HSC 1993

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0.06 UTI
0.0
CN
0.16
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.16 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1993 is a sparse, very loose object of very low 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.

Distant 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 – 116.226 -32.62 0.308 -3.463 5.05 62.834
Hunt & Reffert 2024 116.251 -32.597 0.313 -3.483 5.087 63.376
Cavallo et al. 2024 116.175 -32.624 0.314 – – –
Hunt & Reffert 2023 116.251 -32.597 0.313 -3.483 5.087 63.376

💡 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 – – – – – 184* – –
Cavallo et al. 2024 3.80 3.13 – 275 0.150 – – –
Hunt & Reffert 2023 3.04 2.73 1.86 541 – – – –

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

Visualization

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