UBC 1591

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0.58 UTI
0.3
CN
1.0
Cdens
1.0
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 6.7 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1591 is a poorly populated, very dense object of very high 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, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

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 99999– 204.024 -64.654 0.399 -5.415 -2.07 –
Hu & Soubiran 2025 204.057 -64.641 – – – –
Hunt & Reffert 2024 204.054 -64.646 0.405 -5.412 -2.046 -39.231
Cavallo et al. 2024 204.057 -64.641 0.403 – – –
Hunt & Reffert 2023 204.054 -64.646 0.405 -5.412 -2.046 -39.231
Castro-Ginard et al. 2022 204.01 -64.67 0.4 -5.41 -2.08 –

💡 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] Bfrac BSS
UCC 99999– 2.26 1.68 1.37 385 -0.065 405 – –
Hu & Soubiran 2025 – – – – -0.270(5) – – –
Hunt & Reffert 2024 – – – – – 405(1) – –
Cavallo et al. 2024 2.06 1.70 – 661 0.140 – – –
Hunt & Reffert 2023 2.26 1.68 1.37 385 – – – –
Castro-Ginard et al. 2022 2.71 1.22 – 170 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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