CWNU 2001

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0.40 UTI
0.25
CN
0.87
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.4 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.87 Dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2001 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster (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– 331.852 58.585 0.438 -4.516 -3.465 -49.728
Hunt & Reffert 2024 331.852 58.571 0.432 -4.487 -3.454 -49.38
Cavallo et al. 2024 331.85 58.61 0.438 – – –
Hunt & Reffert 2023 331.852 58.571 0.432 -4.487 -3.454 -49.38
He et al. 2023 331.85 58.587 0.448 -4.519 -3.46 -49.38

💡 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– 2.11 4.3 1.81 158 0.510 202 – –
Hunt & Reffert 2024 – – – – – 202(1) – –
Cavallo et al. 2024 2.52 4.24 – 158 0.510 – – –
Hunt & Reffert 2023 2.11 4.47 1.81 147 – – – –
He et al. 2023 2.00 4.30 – 398 – – – –

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

Visualization

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