CWNU 1684

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0.26 UTI
0.0
CN
0.32
Cdens
0.5
CC3
0.25
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 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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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.

Liu et al. (2025)
Classified as primordial binary cluster 109 along with HSC_1421.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P8, along with HSC_1421.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

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– 1.625 1.595 1.38 66 0.148 219 – –
Liu et al. 2025 2.90 0.56 – 56 – – – –
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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