CWNU 1397

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0.31 UTI
0.34
CN
0.33
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.7 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1397 is a poorly populated, loose object of low 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 absorption and age parameters (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– 299.103 34.177 0.405 -2.051 -5.918 0.969
Hunt & Reffert 2024 299.092 34.231 0.399 -2.057 -5.908 –
Cavallo et al. 2024 299.103 34.168 0.402 – – –
Hunt & Reffert 2023 299.092 34.231 0.399 -2.057 -5.908 –
He et al. 2023 299.083 34.161 0.409 -2.052 -5.911 –

💡 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– 2.54 1.41 1.44 20 0.490 158 – –
Hunt & Reffert 2024 – – – – – 158(1) – –
Cavallo et al. 2024 2.54 1.83 – 49 0.490 – – –
Hunt & Reffert 2023 2.38 1.41 1.44 20 – – – –
He et al. 2023 2.75 0.10 – 1 – – – –

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

Visualization

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