CWNU 1427

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0.55 UTI
0.48
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.8 [N/pc2]
  • CN 0.48 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 1427 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 high extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 255.247 -39.594 0.416 -0.63 -1.462 -34.501
Hunt & Reffert 2024 255.275 -39.592 0.416 -0.616 -1.466 -36.0
Cavallo et al. 2024 255.229 -39.572 0.415 – – –
Hunt & Reffert 2023 255.275 -39.592 0.416 -0.616 -1.466 -36.0
He et al. 2023 255.243 -39.596 0.424 -0.597 -1.461 -39.03

💡 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– 2.25 4.98 2.48 120 0.150 829 – –
Hunt & Reffert 2024 – – – – – 829(1) – –
Cavallo et al. 2024 2.56 4.75 – 95 0.150 – – –
Hunt & Reffert 2023 2.25 4.98 2.48 120 – – – –
He et al. 2023 2.04 5.00 – 251 – – – –

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

Visualization

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