CWNU 2569

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0.48 UTI
0.4
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 9.7 [N/pc2]
  • CN 0.4 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2569 is a poorly populated, very dense object of intermediate 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, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported 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– 267.116 -27.397 0.416 0.883 0.477 -40.364
Hunt & Reffert 2024 267.12 -27.409 0.417 0.856 0.484 -40.363
Cavallo et al. 2024 267.108 -27.396 0.43 – – –
Hunt & Reffert 2023 267.12 -27.409 0.417 0.856 0.484 -40.363
He et al. 2023 267.112 -27.403 0.423 0.867 0.477 -18.06

💡 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– 2.04 4.55 2.35 79 -0.790 457 – –
Hunt & Reffert 2024 – – – – – 457(1) – –
Cavallo et al. 2024 1.44 4.59 – 191 -0.790 – – –
Hunt & Reffert 2023 2.23 4.29 2.35 38 – – – –
He et al. 2023 2.04 4.55 – 79 – – – –

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

Visualization

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