HSC 1590

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0.22 UTI
0.0
CN
0.09
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 21.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1590 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively 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.
Relatively close 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 – 99.209 12.187 0.874 -1.387 -3.193 42.062
Hu & Soubiran 2025 99.216 12.16 – – – –
Zhang et al. 2024 99.227 12.184 – – – –
Hunt & Reffert 2024 99.227 12.184 0.873 -1.461 -3.116 19.819
Cavallo et al. 2024 99.216 12.16 0.873 – – –
Hunt & Reffert 2023 99.227 12.184 0.873 -1.461 -3.116 19.819

💡 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
Hu & Soubiran 2025 – – – – -0.130* – – –
Zhang et al. 2024 – – – – -0.256* – – –
Hunt & Reffert 2024 – – – – – 70* – –
Cavallo et al. 2024 0.99 1.39 – 1023 -0.300 – – –
Hunt & Reffert 2023 1.05 0.94 0.96 335 – – – –

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

Visualization

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