CWNU 1753

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0.27 UTI
0.25
CN
0.21
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1753 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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– 297.734 27.442 0.463 -3.236 -6.254 4.501
Hunt & Reffert 2024 297.727 27.432 0.449 -3.247 -6.229 3.6
Cavallo et al. 2024 297.883 27.715 0.452 – – –
Hunt & Reffert 2023 297.727 27.432 0.449 -3.247 -6.229 3.6
He et al. 2023 297.732 27.456 0.478 -3.236 -6.257 -3.6

💡 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– 1.91 1.76 1.81 105 0.210 125 – –
Hunt & Reffert 2024 – – – – – 125(1) – –
Cavallo et al. 2024 1.87 1.76 – 170 0.210 – – –
Hunt & Reffert 2023 2.02 1.68 1.81 105 – – – –
He et al. 2023 1.91 1.90 – 71 – – – –

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

Visualization

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