CWNU 153

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0.47 UTI
0.35
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 9.6 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 153 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied 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– 302.058 23.164 0.625 -0.398 -5.185 –
Hunt & Reffert 2024 302.064 23.164 0.6 -0.455 -5.182 –
Cavallo et al. 2024 302.043 23.154 0.612 – – –
Hunt & Reffert 2023 302.064 23.164 0.6 -0.455 -5.182 –
He et al. 2022 302.067 23.161 0.61 -0.41 -5.14 –

💡 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– 1.52 1.5 0.46 170 0.733 167 – –
Hunt & Reffert 2024 – – – – – 167(1) – –
Cavallo et al. 2024 1.51 1.36 – 170 0.550 – – –
Hunt & Reffert 2023 1.52 1.60 0.46 127 – – – –
He et al. 2022 1.58 1.50 – 398 0.916 – – –

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

Visualization

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