CWNU 2683

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0.33 UTI
0.0
CN
0.76
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.76 Dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2683 is a sparse, 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 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– 99.914 7.342 0.414 -0.691 -0.708 –
Hunt & Reffert 2024 99.913 7.333 0.424 -0.696 -0.69 –
Cavallo et al. 2024 99.907 7.346 0.425 – – –
Hunt & Reffert 2023 99.913 7.333 0.424 -0.696 -0.69 –
He et al. 2023 99.932 7.342 0.426 -0.684 -0.707 95.73

💡 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– 2.57 1.37 0.93 241 0.450 155 – –
Hunt & Reffert 2024 – – – – – 155(1) – –
Cavallo et al. 2024 2.59 1.04 – 245 0.450 – – –
Hunt & Reffert 2023 2.20 1.37 0.93 241 – – – –
He et al. 2023 2.57 1.85 – 100 – – – –

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

Visualization

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