CWNU 459

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0.36 UTI
0.45
CN
0.21
Cdens
0.75
CC3
0.25
Clit
0.96
Cdup
Radius (P>50% members) 7.6 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.96 Unique

Overview

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CWNU 459 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It is poorly studied in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Massive Metal-rich 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 – 347.946 60.97 0.334 -4.44 -1.789 -68.975
Hunt & Reffert 2024 348.054 60.97 0.336 -4.422 -1.799 -55.471
Cavallo et al. 2024 347.921 61.013 0.336 – – –
Hunt & Reffert 2023 348.054 60.97 0.336 -4.422 -1.799 -55.471
He et al. 2022 348.048 61.037 0.34 -4.44 -1.78 –

💡 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 – – – – – 1172* – –
Cavallo et al. 2024 2.67 2.36 – 27 0.300 – – –
Hunt & Reffert 2023 2.73 2.27 2.20 19 – – – –
He et al. 2022 2.40 1.98 – 63 0.916 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0425 4.4 348.56 61.22 0.35 -4.43 -1.86 – 0.29
CWWDL 2573 2.2 347.57 60.95 0.32 -4.13 -1.97 – 0.03

💡 Note: The % column shows the percentage of members that CWNU 459 shares with each listed object.

Visualization

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