CWNU 1528

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0.52 UTI
0.48
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.48 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1528 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Metal-poor Young

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 – 224.491 -58.057 0.421 -4.861 -2.908 -49.695
Hunt & Reffert 2024 224.49 -58.055 0.414 -4.872 -2.938 -49.678
Cavallo et al. 2024 224.503 -58.069 0.418 – – –
Hunt & Reffert 2023 224.49 -58.055 0.414 -4.872 -2.938 -49.678
He et al. 2023 224.491 -58.057 0.421 -4.865 -2.905 -49.28

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 770* – –
Cavallo et al. 2024 1.51 4.05 – 234 -0.800 – – –
Hunt & Reffert 2023 2.19 3.85 2.61 66 – – – –
He et al. 2023 2.24 4.10 – 56 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 9622 75.0 224.49 -58.06 0.42 -4.87 -2.94 -49.7 0.01

💡 Note: The % column shows the percentage of members that CWNU 1528 shares with each listed object.

Visualization

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