CWNU 2404

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0.30 UTI
0.38
CN
0.45
Cdens
0.75
CC3
0.25
Clit
0.71
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.38 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.71 Likely unique

Overview

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CWNU 2404 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

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– 318.981 48.695 0.34 -4.235 -4.661 -28.098
Hunt & Reffert 2024 318.998 48.717 0.327 -4.205 -4.648 -28.102
Cavallo et al. 2024 318.979 48.709 0.329 – – –
Hunt & Reffert 2023 318.998 48.717 0.327 -4.205 -4.648 -28.102
He et al. 2023 318.994 48.709 0.348 -4.217 -4.663 -57.14

💡 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– 2.79 2.65 2.17 38 0.530 365 – –
Hunt & Reffert 2024 – – – – – 365(1) – –
Cavallo et al. 2024 3.16 2.68 – 19 0.530 – – –
Hunt & Reffert 2023 2.79 2.53 2.17 38 – – – –
He et al. 2023 2.63 2.65 – 200 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Basel 15 28.9 318.99 48.8 0.31 -4.12 -4.58 – 0.19

💡 Note: The % column shows the percentage of members that CWNU 2404 shares with each listed object.

Visualization

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