CWNU 2564

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0.53 UTI
0.5
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.1 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2564 is a moderately populated, very dense object of intermediate 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, young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction 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 – 342.622 61.217 0.223 -3.455 -1.987 –
Hunt & Reffert 2024 342.623 61.223 0.238 -3.453 -1.971 –
Cavallo et al. 2024 342.59 61.219 0.23 – – –
Hunt & Reffert 2023 342.623 61.223 0.238 -3.453 -1.971 –
He et al. 2023 342.626 61.22 0.228 -3.454 -1.988 –

💡 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 – – – – – 965* – –
Cavallo et al. 2024 3.87 3.87 – 72 0.450 – – –
Hunt & Reffert 2023 4.03 4.28 2.40 35 – – – –
He et al. 2023 5.37 5.00 – 2 – – – –

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

Visualization

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