CWNU 446

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0.56 UTI
0.57
CN
1.0
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.8 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 446 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a 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.
Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 340.194 65.313 1.053 -0.314 -2.569 -32.69
Hunt & Reffert 2024 340.173 65.289 1.024 -0.331 -2.545 -33.234
Cavallo et al. 2024 340.161 65.324 1.02 – – –
Hunt & Reffert 2023 340.173 65.289 1.024 -0.331 -2.545 -33.234
He et al. 2022 339.949 65.418 1.071 -0.346 -2.555 –
He et al. 2022 340.135 65.305 1.05 -0.38 -2.64 -50.2

💡 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 – – – – – 145* – –
Cavallo et al. 2024 1.10 1.75 – 9 0.010 – – –
Hunt & Reffert 2023 0.95 1.78 1.74 4 – – – –
He et al. 2022 – 2.10 – 6 – – – –
He et al. 2022 0.69 2.28 – 25 -0.642 – – –

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

Visualization

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