CWNU 1336

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0.45 UTI
0.25
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 6.0 [N/pc2]
  • CN 0.25 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 1336 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a very metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

Cavallo et al. (2024)
Bronze 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– 305.417 34.312 0.341 -2.26 -4.4 123.59
Hunt & Reffert 2024 305.415 34.31 0.339 -2.264 -4.378 123.625
Cavallo et al. 2024 305.406 34.325 0.344 – – –
Hunt & Reffert 2023 305.415 34.31 0.339 -2.264 -4.378 123.625
He et al. 2023 305.415 34.318 0.349 -2.261 -4.399 –

💡 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– 2.7 4.91 2.6 14 1.170 764 – –
Hunt & Reffert 2024 – – – – – 764(1) – –
Cavallo et al. 2024 3.31 4.16 – 26 1.170 – – –
Hunt & Reffert 2023 2.70 4.91 2.60 14 – – – –
He et al. 2023 2.69 5.60 – 4 – – – –

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

Visualization

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