CWNU 1308

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0.55 UTI
0.6
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 8.2 [N/pc2]
  • CN 0.6 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1308 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by 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)
Silver 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– 276.14 -14.079 0.329 -0.654 -2.036 38.803
Hunt & Reffert 2024 276.127 -14.052 0.313 -0.633 -2.046 43.029
Cavallo et al. 2024 276.147 -14.089 0.316 – – –
Hunt & Reffert 2023 276.127 -14.052 0.313 -0.633 -2.046 43.029
He et al. 2023 276.154 -14.089 0.333 -0.639 -2.031 38.8

💡 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– 2.57 4.1 2.61 63 -0.480 962 – –
Hunt & Reffert 2024 – – – – – 962(1) – –
Cavallo et al. 2024 1.85 4.23 – 65 -0.480 – – –
Hunt & Reffert 2023 2.81 3.85 2.61 43 – – – –
He et al. 2023 2.57 4.10 – 63 – – – –

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

Visualization

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