CWNU 1749

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0.32 UTI
0.29
CN
0.45
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.3 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1749 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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– 2.491 60.387 0.438 -2.163 -1.391 -42.123
Hunt & Reffert 2024 2.489 60.414 0.437 -2.146 -1.4 -41.292
Cavallo et al. 2024 2.448 60.403 0.439 – – –
Hunt & Reffert 2023 2.489 60.414 0.437 -2.146 -1.4 -41.292
He et al. 2023 2.482 60.382 0.438 -2.164 -1.377 –

💡 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– 2.14 1.12 0.69 167 0.170 143 – –
Hunt & Reffert 2024 – – – – – 143(1) – –
Cavallo et al. 2024 1.93 1.03 – 245 0.170 – – –
Hunt & Reffert 2023 2.17 1.12 0.69 167 – – – –
He et al. 2023 2.14 1.60 – 50 – – – –

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

Visualization

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