CWNU 201

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0.45 UTI
0.29
CN
0.48
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 12.1 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 0.48 Loose
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 201 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Close Moderate 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 – 95.409 -10.302 1.018 -3.575 -0.871 34.538
Hu & Soubiran 2025 95.459 -10.357 – – – –
Hunt & Reffert 2024 95.378 -10.283 1.004 -3.519 -0.832 33.575
Cavallo et al. 2024 95.459 -10.357 1.004 – – –
Hunt & Reffert 2023 95.378 -10.283 1.004 -3.519 -0.832 33.575
He et al. 2022 95.382 -10.284 1.018 -3.594 -0.867 –
He et al. 2022 95.393 -10.278 1.02 -3.59 -0.87 39.9

💡 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 – – – – -0.220* – – –
Hunt & Reffert 2024 – – – – – 57* – –
Cavallo et al. 2024 0.92 1.88 – 871 -0.070 – – –
Hunt & Reffert 2023 0.95 1.59 1.30 1038 – – – –
He et al. 2022 – 2.10 – 501 – – – –
He et al. 2022 0.83 1.74 – 1995 -1.335 – – –

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

Visualization

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