CWNU 482

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0.35 UTI
0.0
CN
0.77
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.77 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 482 is a sparse, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate 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 – 272.54 -22.382 0.657 -0.528 -1.56 22.335
Hunt & Reffert 2024 272.482 -22.283 0.656 -0.522 -1.54 12.143
Cavallo et al. 2024 272.512 -22.337 0.653 – – –
Hunt & Reffert 2023 272.482 -22.283 0.656 -0.522 -1.54 12.143
He et al. 2022 272.603 -22.361 0.67 -0.55 -1.54 –

💡 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 – – – – – 216* – –
Cavallo et al. 2024 1.24 2.48 – 11 -0.500 – – –
Hunt & Reffert 2023 1.46 1.93 0.88 23 – – – –
He et al. 2022 1.58 2.34 – 158 0.862 – – –

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

Visualization

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