CWNU 480

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0.51 UTI
0.54
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.5 [N/pc2]
  • CN 0.54 Moderately 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 480 is a moderately populated, 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 metal-rich, very young cluster (see Parameters). It is poorly studied in the literature.

Palma et al. (2025)
Part of multiple system G96, along with CWNU_1866, Gulliver_58 and UBC_522.

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– 193.498 -61.99 0.42 -4.202 -1.176 -20.449
Hunt & Reffert 2024 193.485 -62.0 0.416 -4.215 -1.173 -18.188
Cavallo et al. 2024 193.538 -61.943 0.417 – – –
Hunt & Reffert 2023 193.485 -62.0 0.416 -4.215 -1.173 -18.188
He et al. 2022 193.492 -62.006 0.42 -4.18 -1.18 –

💡 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– 2.28 3.7 2.94 11 0.566 789 – –
Hunt & Reffert 2024 – – – – – 789(1) – –
Cavallo et al. 2024 1.99 3.70 – 26 0.520 – – –
Hunt & Reffert 2023 2.28 3.53 2.94 11 – – – –
He et al. 2022 3.63 4.44 – 5 0.611 – – –

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

Visualization

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