CWNU 2812

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0.52 UTI
0.35
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.6 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2812 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very 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)
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– 228.485 -55.529 0.277 -4.938 -3.732 -73.484
Hunt & Reffert 2024 228.464 -55.531 0.275 -4.938 -3.768 –
Cavallo et al. 2024 228.455 -55.513 0.292 – – –
Hunt & Reffert 2023 228.464 -55.531 0.275 -4.938 -3.768 –
He et al. 2023 228.493 -55.524 0.329 -4.909 -3.711 -73.07

💡 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– 2.89 5.37 1.76 627 0.150 1728 – –
Hunt & Reffert 2024 – – – – – 1728(1) – –
Cavallo et al. 2024 4.31 5.37 – 135 0.150 – – –
Hunt & Reffert 2023 2.89 5.86 1.76 627 – – – –
He et al. 2023 2.45 4.65 – 2239 – – – –

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

Visualization

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