CWNU 406

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0.43 UTI
0.28
CN
0.38
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 12.9 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.38 Loose
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 406 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Close Low 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 – 91.272 20.84 0.982 1.568 -2.266 -1.082
Zhang et al. 2024 91.399 20.814 – – – –
Hunt & Reffert 2024 91.399 20.814 0.98 1.612 -2.281 -4.574
Cavallo et al. 2024 91.241 20.948 0.976 – – –
Hunt & Reffert 2023 91.399 20.814 0.98 1.612 -2.281 -4.574
He et al. 2022 91.265 20.817 0.982 1.555 -2.232 –
He et al. 2022 91.319 20.841 0.98 1.59 -2.25 –

💡 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
Zhang et al. 2024 – – – – -0.076* – – –
Hunt & Reffert 2024 – – – – – 149* – –
Cavallo et al. 2024 0.99 0.62 – 479 0.110 – – –
Hunt & Reffert 2023 0.96 0.66 0.75 181 – – – –
He et al. 2022 – 0.85 – 79 – – – –
He et al. 2022 1.10 1.20 – 63 -0.642 – – –

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

Visualization

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