CWNU 1387

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0.40 UTI
0.26
CN
1.0
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 9.8 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1387 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very 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)
Wood 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– 281.686 -2.938 0.411 -1.264 -2.063 40.268
Hunt & Reffert 2024 281.697 -2.917 0.408 -1.255 -2.049 40.28
Cavallo et al. 2024 281.668 -2.94 0.411 – – –
Hunt & Reffert 2023 281.697 -2.917 0.408 -1.255 -2.049 40.28
He et al. 2023 281.688 -2.936 0.411 -1.261 -2.064 40.27

💡 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– 2.23 5.79 2.33 67 0.180 554 – –
Hunt & Reffert 2024 – – – – – 554(1) – –
Cavallo et al. 2024 3.66 4.86 – 44 0.180 – – –
Hunt & Reffert 2023 2.23 5.79 2.33 67 – – – –
He et al. 2023 2.14 6.30 – 126 – – – –

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

Visualization

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