HSC 2090

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0.11 UTI
0.0
CN
0.28
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.28 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2090 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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 High 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 – 131.568 -39.789 0.249 -2.85 3.432 42.997
Hunt & Reffert 2024 131.577 -39.807 0.239 -2.82 3.46 36.311
Cavallo et al. 2024 131.572 -39.789 0.239 – – –
Hunt & Reffert 2023 131.577 -39.807 0.239 -2.82 3.46 36.311

💡 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 – – – – – 534* – –
Cavallo et al. 2024 3.66 4.31 – 339 -0.110 – – –
Hunt & Reffert 2023 3.76 4.24 2.00 231 – – – –

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

Visualization

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