CWNU 2778

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0.40 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2778 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, 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)
Silver 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– 252.654 -41.82 0.346 -2.331 -3.744 -27.906
Hunt & Reffert 2024 252.656 -41.826 0.344 -2.328 -3.753 -31.705
Cavallo et al. 2024 252.636 -41.822 0.344 – – –
Hunt & Reffert 2023 252.656 -41.826 0.344 -2.328 -3.753 -31.705
He et al. 2023 252.666 -41.819 0.396 -2.331 -3.763 -33.43

💡 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– 2.34 4.27 2.71 324 -0.070 1902 – –
Hunt & Reffert 2024 – – – – – 1902(1) – –
Cavallo et al. 2024 2.34 4.27 – 324 -0.070 – – –
Hunt & Reffert 2023 2.67 4.61 2.71 209 – – – –
He et al. 2023 2.34 3.80 – 1122 – – – –

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

Visualization

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