CWNU 141

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0.60 UTI
0.5
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.7 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 141 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below 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.
Relatively 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 – 247.956 -52.87 0.572 -2.888 -3.438 -39.473
Hunt & Reffert 2024 247.939 -52.881 0.564 -2.909 -3.437 -39.934
Cavallo et al. 2024 247.985 -52.862 0.565 – – –
Hunt & Reffert 2023 247.939 -52.881 0.564 -2.909 -3.437 -39.934
He et al. 2022 247.974 -52.878 0.57 -2.89 -3.44 -37.9

💡 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
Hunt & Reffert 2024 – – – – – 374* – –
Cavallo et al. 2024 1.35 1.53 – 91 -0.460 – – –
Hunt & Reffert 2023 1.65 1.00 1.26 72 – – – –
He et al. 2022 1.41 1.20 – 158 -0.419 – – –

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

Visualization

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