CWNU 2419

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0.37 UTI
0.0
CN
0.59
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.59 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2419 is a sparse, moderately dense 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 near-solar metallicity, young cluster (see Parameters). It was recently reported 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 – 176.281 -63.191 0.395 -7.07 0.565 –
Hunt & Reffert 2024 176.188 -63.225 0.402 -7.064 0.575 -23.538
Cavallo et al. 2024 176.325 -63.194 0.402 – – –
Hunt & Reffert 2023 176.188 -63.225 0.402 -7.064 0.575 -23.538
He et al. 2023 176.368 -63.195 0.404 -7.055 0.533 -23.89

💡 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 – – – – – 206* – –
Cavallo et al. 2024 2.03 1.10 – 100 -0.380 – – –
Hunt & Reffert 2023 2.25 0.89 0.93 55 – – – –
He et al. 2023 2.29 1.05 – 50 – – – –

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

Visualization

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