CWNU 1439

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0.56 UTI
0.45
CN
0.87
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.3 [N/pc2]
  • CN 0.45 Poorly populated
  • Cdens 0.87 Dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1439 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, 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)
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 99999– 214.865 -62.247 0.289 -6.042 -2.329 -78.768
Hunt & Reffert 2024 214.949 -62.203 0.289 -6.035 -2.341 –
Cavallo et al. 2024 214.874 -62.234 0.289 – – –
Hunt & Reffert 2023 214.949 -62.203 0.289 -6.035 -2.341 –
He et al. 2023 214.855 -62.238 0.312 -6.049 -2.358 –

💡 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– 3.19 4.16 2.53 97 0.510 1183 – –
Hunt & Reffert 2024 – – – – – 1183(1) – –
Cavallo et al. 2024 3.19 3.75 – 120 0.510 – – –
Hunt & Reffert 2023 3.06 4.16 2.53 97 – – – –
He et al. 2023 3.98 4.60 – 3 – – – –

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

Visualization

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