UBC 566

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0.70 UTI
0.87
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.8 [arcmin]
  • CN 0.87 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 566 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a very massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Very high extinction Very massive Near-solar metallicity Young

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 – 263.669 -33.094 0.385 0.305 -0.509 -9.514
Hunt & Reffert 2024 263.68 -33.099 0.39 0.303 -0.494 -9.907
Cavallo et al. 2024 263.666 -33.126 0.389 – – –
Hunt & Reffert 2023 263.68 -33.099 0.39 0.303 -0.494 -9.907
Cantat-Gaudin et al. 2020 263.681 -33.102 0.378 0.252 -0.517 –
Castro-Ginard et al. 2020 263.687 -33.112 0.386 0.238 -0.513 –

💡 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 – – – – – 9379* – –
Cavallo et al. 2024 2.12 5.46 – 19 -0.460 – – –
Hunt & Reffert 2023 2.36 4.91 2.88 32 – – – –

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

Visualization

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