CWNU 1684

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0.28 UTI
0.0
CN
0.32
Cdens
0.5
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 1.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.32 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1684 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (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– 85.407 28.2 0.61 1.007 -1.931 –
Zhang et al. 2024 85.359 28.197 – – – –
Hunt & Reffert 2024 85.359 28.197 0.62 1.012 -1.937 –
Cavallo et al. 2024 85.375 28.173 0.62 – – –
Hunt & Reffert 2023 85.359 28.197 0.62 1.012 -1.937 –
He et al. 2023 85.42 28.169 0.62 1.01 -1.934 –

💡 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– 1.58 1.7 1.38 76 0.148 219 – –
Zhang et al. 2024 – – – – -0.263(1) – – –
Hunt & Reffert 2024 – – – – – 219(1) – –
Cavallo et al. 2024 1.67 1.49 – 174 0.560 – – –
Hunt & Reffert 2023 1.51 1.73 1.38 76 – – – –
He et al. 2023 1.58 1.70 – 20 – – – –

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

Visualization

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