CWNU 2363

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0.46 UTI
0.32
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 17.6 [N/pc2]
  • CN 0.32 Poorly populated
  • 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 2363 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young 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– 212.813 -61.137 0.388 -3.881 -2.315 –
Hunt & Reffert 2024 212.818 -61.136 0.386 -3.881 -2.325 –
Cavallo et al. 2024 212.819 -61.133 0.38 – – –
Hunt & Reffert 2023 212.818 -61.136 0.386 -3.881 -2.325 –
He et al. 2023 212.814 -61.138 0.388 -3.863 -2.309 -40.72

💡 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– 2.45 3.58 2.29 7 0.130 556 – –
Hunt & Reffert 2024 – – – – – 556(1) – –
Cavallo et al. 2024 2.36 3.56 – 7 0.130 – – –
Hunt & Reffert 2023 2.46 3.58 2.29 6 – – – –
He et al. 2023 2.45 4.05 – 11 – – – –

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

Visualization

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