CWNU 42

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0.40 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 42 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near 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.
Relatively 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 – 318.276 46.068 0.408 0.062 -1.674 –
Hunt & Reffert 2024 318.273 46.083 0.398 0.018 -1.699 -11.411
Cavallo et al. 2024 318.241 46.052 0.4 – – –
Hunt & Reffert 2023 318.273 46.083 0.398 0.018 -1.699 -11.411
He et al. 2022 318.251 46.07 0.41 0.06 -1.64 –

💡 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 – – – – – 256* – –
Cavallo et al. 2024 2.40 1.66 – 178 -0.050 – – –
Hunt & Reffert 2023 2.30 1.44 2.47 270 – – – –
He et al. 2022 2.19 1.56 – 32 0.274 – – –

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

Visualization

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