CWNU 2284

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0.32 UTI
0.28
CN
0.06
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.3 [N/pc2]
  • CN 0.28 Poorly populated
  • Cdens 0.06 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2284 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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– 109.388 -9.548 0.351 -2.207 2.032 –
Hunt & Reffert 2024 109.347 -9.454 0.34 -2.166 2.055 64.443
Cavallo et al. 2024 109.356 -9.468 0.341 – – –
Hunt & Reffert 2023 109.347 -9.454 0.34 -2.166 2.055 64.443
He et al. 2023 109.459 -9.74 0.352 -2.205 2.05 103.57

💡 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– 2.53 0.91 2.01 158 0.070 175 – –
Hunt & Reffert 2024 – – – – – 175(1) – –
Cavallo et al. 2024 2.55 0.91 – 158 0.070 – – –
Hunt & Reffert 2023 2.53 0.76 2.01 304 – – – –
He et al. 2023 2.51 1.00 – 32 – – – –

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

Visualization

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