CWNU 1512

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0.41 UTI
0.31
CN
1.0
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.8 [N/pc2]
  • CN 0.31 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 1512 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 moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 105.007 -3.967 0.378 -0.641 -1.182 42.1
Hunt & Reffert 2024 105.012 -3.972 0.376 -0.636 -1.188 42.117
Cavallo et al. 2024 105.005 -3.973 0.374 – – –
Hunt & Reffert 2023 105.012 -3.972 0.376 -0.636 -1.188 42.117
He et al. 2023 104.988 -3.987 0.386 -0.636 -1.15 –

💡 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– 2.47 1.87 1.68 234 0.300 279 – –
Hunt & Reffert 2024 – – – – – 279(1) – –
Cavallo et al. 2024 2.20 1.87 – 234 0.300 – – –
Hunt & Reffert 2023 2.47 1.95 1.68 252 – – – –
He et al. 2023 2.88 0.05 – 1 – – – –

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

Visualization

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