CWNU 1639

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0.27 UTI
0.0
CN
0.98
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 4.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.98 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1639 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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.

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– 331.562 59.525 0.348 -1.791 -2.465 -52.44
Hunt & Reffert 2024 331.548 59.518 0.352 -1.786 -2.456 -52.382
Cavallo et al. 2024 331.579 59.518 0.352 – – –
Hunt & Reffert 2023 331.548 59.518 0.352 -1.786 -2.456 -52.382
He et al. 2023 331.58 59.512 0.359 -1.8 -2.464 -52.86

💡 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– 2.83 2.46 0.97 240 0.620 263 – –
Hunt & Reffert 2024 – – – – – 263(1) – –
Cavallo et al. 2024 2.92 2.21 – 240 0.620 – – –
Hunt & Reffert 2023 2.83 2.46 0.97 143 – – – –
He et al. 2023 2.57 2.70 – 251 – – – –

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

Visualization

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