CWNU 1310

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0.49 UTI
0.51
CN
0.68
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 3.4 [N/pc2]
  • CN 0.51 Moderately populated
  • Cdens 0.68 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1310 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 300.122 32.796 0.245 -3.14 -5.065 -1.431
Hunt & Reffert 2024 300.086 32.793 0.239 -3.138 -5.055 31.61
Cavallo et al. 2024 300.121 32.8 0.239 – – –
Hunt & Reffert 2023 300.086 32.793 0.239 -3.138 -5.055 31.61
He et al. 2023 300.135 32.787 0.243 -3.145 -5.069 -1.43

💡 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– 3.63 3.29 2.23 224 0.360 376 – –
Hunt & Reffert 2024 – – – – – 376(1) – –
Cavallo et al. 2024 3.27 3.29 – 224 0.360 – – –
Hunt & Reffert 2023 3.98 3.23 2.23 102 – – – –
He et al. 2023 3.63 3.45 – 398 – – – –

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

Visualization

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