UBC 564

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0.55 UTI
0.26
CN
0.78
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 3.9 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.78 Dense
  • CC3 1.0 Very high quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
UBC 564 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Part of multiple system G170, along with Ruprecht_127, HSC_2912, CWNU_50 and HSC_2921.

Cavallo et al. (2024)
Silver 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– 263.992 -34.639 0.394 -0.253 -1.696 -5.394
Hunt & Reffert 2024 264.01 -34.636 0.405 -0.269 -1.675 -5.375
Celli et al. 2024 263.999 -34.645 – – – –
Cavallo et al. 2024 263.994 -34.637 0.405 – – –
Hunt & Reffert 2023 264.01 -34.636 0.405 -0.269 -1.675 -5.375
Cantat-Gaudin et al. 2020 263.999 -34.645 0.373 -0.234 -1.719 –
Castro-Ginard et al. 2020 264.005 -34.649 0.373 -0.225 -1.725 –

💡 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– 2.37 3.28 1.56 28 -0.500 622 – –
Hunt & Reffert 2024 – – – – – 541(1) – –
Celli et al. 2024 – – – 26 – 703 – –
Cavallo et al. 2024 1.36 3.86 – 34 -0.500 – – –
Hunt & Reffert 2023 2.37 3.28 1.56 29 – – – –
Cantat-Gaudin et al. 2020 2.40 3.02 – 26 – – – –

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

Visualization

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