CWNU 1405

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0.47 UTI
0.34
CN
0.53
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.6 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.53 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1405 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (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– 167.14 -59.441 0.203 -7.268 2.862 -0.85
Hunt & Reffert 2024 167.134 -59.442 0.195 -7.27 2.851 –
Cavallo et al. 2024 167.159 -59.435 0.195 – – –
Hunt & Reffert 2023 167.134 -59.442 0.195 -7.27 2.851 –
He et al. 2023 167.136 -59.444 0.212 -7.274 2.85 –

💡 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– 5.23 2.02 1.74 77 -0.290 351 – –
Hunt & Reffert 2024 – – – – – 351(1) – –
Cavallo et al. 2024 3.39 1.85 – 224 -0.290 – – –
Hunt & Reffert 2023 5.23 2.02 1.74 77 – – – –
He et al. 2023 5.50 2.70 – 6 – – – –

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

Visualization

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