CWNU 1145

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0.26 UTI
0.29
CN
0.16
Cdens
0.25
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 0.8 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 0.16 Very loose
  • CC3 0.25 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1145 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied 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– 75.797 39.931 0.947 -0.491 -3.009 -20.96
Zhang et al. 2024 75.727 39.946 – – – –
Hunt & Reffert 2024 75.726 39.946 0.9 -0.5 -3.026 -24.034
Cavallo et al. 2024 76.035 39.847 0.899 – – –
Hunt & Reffert 2023 75.726 39.946 0.9 -0.5 -3.026 -24.034
He et al. 2022 75.654 39.999 0.977 -0.488 -2.946 –

💡 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– 1.08 0.72 1.35 86 0.051 54 – –
Zhang et al. 2024 – – – – -0.167(1) – – –
Hunt & Reffert 2024 – – – – – 54(1) – –
Cavallo et al. 2024 1.12 0.54 – 398 0.270 – – –
Hunt & Reffert 2023 1.04 0.72 1.35 86 – – – –
He et al. 2022 – 1.10 – 50 – – – –

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

Visualization

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