CWNU 252

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0.57 UTI
0.47
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.5 [arcmin]
  • CN 0.47 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 252 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 metallicity parameter (see Parameters). It is poorly studied 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 Low extinction Near-solar metallicity Intermediate age

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 – 185.366 -61.064 0.78 -7.068 -0.671 -20.393
Hu & Soubiran 2025 185.484 -61.05 – – – –
Hunt & Reffert 2024 185.398 -61.072 0.777 -7.055 -0.658 -16.109
Cavallo et al. 2024 185.484 -61.05 0.779 – – –
Hunt & Reffert 2023 185.398 -61.072 0.777 -7.055 -0.658 -16.109
He et al. 2022 185.376 -61.085 0.76 -7.05 -0.72 -3.4

💡 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
Hu & Soubiran 2025 – – – – -0.250* – – –
Hunt & Reffert 2024 – – – – – 123* – –
Cavallo et al. 2024 1.19 0.42 – 501 0.270 – – –
Hunt & Reffert 2023 1.23 0.72 0.83 261 – – – –
He et al. 2022 1.62 1.14 – 100 0.805 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14187 53.2 185.36 -61.07 0.78 -7.04 -0.61 -12.93 0.0

💡 Note: The % column shows the percentage of members that CWNU 252 shares with each listed object.

Visualization

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