CWNU 1468

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0.48 UTI
0.4
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 8.9 [N/pc2]
  • CN 0.4 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 1468 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, young cluster (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– 271.399 -22.818 0.426 -1.113 -2.649 4.41
Hunt & Reffert 2024 271.399 -22.793 0.445 -1.073 -2.667 -3.849
Cavallo et al. 2024 271.391 -22.818 0.442 – – –
Hunt & Reffert 2023 271.399 -22.793 0.445 -1.073 -2.667 -3.849
He et al. 2023 271.39 -22.819 0.442 -1.109 -2.632 -3.83

💡 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– 2.14 3.04 1.9 75 -0.090 359 – –
Hunt & Reffert 2024 – – – – – 359(1) – –
Cavallo et al. 2024 2.23 2.91 – 74 -0.090 – – –
Hunt & Reffert 2023 2.13 3.04 1.90 75 – – – –
He et al. 2023 2.14 3.15 – 126 – – – –

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

Visualization

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