CWNU 475

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0.49 UTI
0.31
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.4 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 475 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 316.167 59.847 0.794 -3.273 -3.546 -4.056
Hunt & Reffert 2024 316.187 59.858 0.777 -3.312 -3.527 -4.001
Cavallo et al. 2024 316.18 59.884 0.799 – – –
Hunt & Reffert 2023 316.187 59.858 0.777 -3.312 -3.527 -4.001
He et al. 2022 316.182 59.839 0.8 -3.3 -3.6 -31.5

💡 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 – – – – – 114* – –
Cavallo et al. 2024 1.31 2.42 – 3 -0.060 – – –
Hunt & Reffert 2023 1.21 2.60 1.50 4 – – – –
He et al. 2022 0.91 2.52 – 316 0.968 – – –

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

Visualization

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