CWNU 463

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0.48 UTI
0.6
CN
0.8
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 9.1 [arcmin]
  • CN 0.6 Moderately populated
  • Cdens 0.8 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 463 is a moderately populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High 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 – 343.259 60.271 0.634 0.622 -2.999 3.107
Hunt & Reffert 2024 343.227 60.277 0.626 0.597 -3.01 3.081
Cavallo et al. 2024 343.236 60.242 0.627 – – –
Hunt & Reffert 2023 343.227 60.277 0.626 0.597 -3.01 3.081
He et al. 2022 343.285 60.275 0.63 0.62 -3.0 –

💡 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 – – – – – 300* – –
Cavallo et al. 2024 1.79 2.83 – 120 0.780 – – –
Hunt & Reffert 2023 1.53 3.22 2.72 99 – – – –
He et al. 2022 2.34 4.44 – 8 -0.642 – – –

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

Visualization

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