CWNU 2580

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0.31 UTI
0.44
CN
0.35
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.7 [N/pc2]
  • CN 0.44 Poorly populated
  • Cdens 0.35 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2580 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, 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– 65.45 45.537 0.377 -0.046 -1.032 32.946
Hunt & Reffert 2024 65.515 45.486 0.353 -0.031 -1.022 32.971
Cavallo et al. 2024 65.405 45.583 0.358 – – –
Hunt & Reffert 2023 65.515 45.486 0.353 -0.031 -1.022 32.971
He et al. 2023 65.384 45.57 0.391 -0.071 -1.018 -20.36

💡 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– 2.56 3.06 2.21 136 0.200 547 – –
Hunt & Reffert 2024 – – – – – 547(1) – –
Cavallo et al. 2024 2.79 3.06 – 63 0.200 – – –
Hunt & Reffert 2023 2.56 2.94 2.21 136 – – – –
He et al. 2023 2.40 3.15 – 141 – – – –

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

Visualization

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