CWNU 182

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0.33 UTI
0.29
CN
0.25
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 17.4 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 182 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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

Close Moderate extinction Near-solar metallicity 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 – 135.916 -43.943 1.047 -8.747 5.779 28.674
Hunt & Reffert 2024 135.849 -43.87 1.063 -8.974 5.719 25.923
Cavallo et al. 2024 136.364 -44.238 1.068 – – –
Hunt & Reffert 2023 135.849 -43.87 1.063 -8.974 5.719 25.923
He et al. 2022 135.841 -43.904 1.043 -8.737 5.797 –
He et al. 2022 136.329 -44.241 1.06 -8.94 5.74 25.5

💡 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 – – – – – 70* – –
Cavallo et al. 2024 1.03 1.60 – 74 0.020 – – –
Hunt & Reffert 2023 0.90 1.43 2.42 106 – – – –
He et al. 2022 – 2.15 – 35 – – – –
He et al. 2022 0.83 1.14 – 794 0.274 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2136 3.4 135.41 -43.24 1.21 -9.51 5.69 15.49 0.1

💡 Note: The % column shows the percentage of members that CWNU 182 shares with each listed object.

Visualization

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