CWNU 1719

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0.57 UTI
0.35
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 18.3 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1719 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (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– 269.954 -21.56 0.316 -0.39 -2.008 94.422
Hunt & Reffert 2024 269.958 -21.558 0.312 -0.394 -1.991 40.696
Cavallo et al. 2024 269.957 -21.556 0.314 – – –
Hunt & Reffert 2023 269.958 -21.558 0.312 -0.394 -1.991 40.696
He et al. 2023 269.956 -21.554 0.324 -0.424 -2.004 -13.05

💡 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– 2.78 4.93 2.29 11 -0.240 1278 – –
Hunt & Reffert 2024 – – – – – 1278(1) – –
Cavallo et al. 2024 2.39 4.93 – 11 -0.240 – – –
Hunt & Reffert 2023 2.78 4.80 2.29 18 – – – –
He et al. 2023 3.24 5.60 – 3 – – – –

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

Visualization

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