CWNU 2767

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0.38 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2767 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Wood 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– 223.742 -60.214 0.339 -3.363 -2.93 -43.768
Hunt & Reffert 2024 223.728 -60.232 0.328 -3.374 -2.951 -43.916
Cavallo et al. 2024 223.741 -60.211 0.328 – – –
Hunt & Reffert 2023 223.728 -60.232 0.328 -3.374 -2.951 -43.916
He et al. 2023 223.746 -60.231 0.337 -3.37 -2.909 -43.77

💡 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– 2.69 5.39 2.83 178 0.540 813 – –
Hunt & Reffert 2024 – – – – – 813(1) – –
Cavallo et al. 2024 3.27 5.08 – 32 0.540 – – –
Hunt & Reffert 2023 2.56 5.39 2.83 373 – – – –
He et al. 2023 2.69 6.45 – 178 – – – –

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

Visualization

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