CWNU 2888

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0.37 UTI
0.0
CN
0.66
Cdens
0.5
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 3.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.66 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2888 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the distance, age, and metallicity parameters (see Parameters). It was recently reported in the literature.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 119 along with UBC_292, and as tidal capture (resonant trapping binary) 128 along with Collinder_272, and of multiple system 40 along with Collinder_272 and UBC_292.

Palma et al. (2025)
Classified as optical pair P364, along with UBC_292.

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– 201.295 -62.298 0.45 -3.947 -0.97 -34.654
Liu et al. 2025 201.33 -62.28 0.45 -4.0 -1.0 -27.53
Hu & Soubiran 2025 201.202 -62.303 – – – –
Hunt & Reffert 2024 201.332 -62.279 0.447 -3.995 -0.997 -27.533
Cavallo et al. 2024 201.202 -62.303 0.448 – – –
Hunt & Reffert 2023 201.332 -62.279 0.447 -3.995 -0.997 -27.533
He et al. 2023 201.281 -62.303 0.453 -3.944 -0.985 –

💡 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– 2.09 1.94 2.51 162 0.000 368 – –
Liu et al. 2025 6.67 0.90 – 102 – – – –
Hu & Soubiran 2025 – – – – -0.180(5) – – –
Hunt & Reffert 2024 – – – – – 368(1) – –
Cavallo et al. 2024 1.89 1.80 – 776 0.180 – – –
Hunt & Reffert 2023 2.09 2.08 2.51 222 – – – –
He et al. 2023 2.09 2.60 – 9 – – – –

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

Visualization

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