CWNU 1541

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0.44 UTI
0.28
CN
0.54
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 2.2 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.54 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1541 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate 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 was recently reported in the literature.
Distant 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 – 135.342 -40.464 0.199 -3.793 2.588 47.35
Hu & Soubiran 2025 135.352 -40.462 – – – –
Hunt & Reffert 2024 135.343 -40.471 0.198 -3.817 2.645 47.43
Cavallo et al. 2024 135.353 -40.462 0.195 – – –
Hunt & Reffert 2023 135.343 -40.471 0.198 -3.817 2.645 47.43
He et al. 2023 135.348 -40.464 0.199 -3.77 2.582 47.28

💡 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
Hu & Soubiran 2025 – – – – -0.210* – – –
Hunt & Reffert 2024 – – – – – 226* – –
Cavallo et al. 2024 3.52 2.35 – 501 -0.670 – – –
Hunt & Reffert 2023 4.38 2.12 1.52 429 – – – –
He et al. 2023 4.27 1.70 – 794 – – – –

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

Visualization

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