CWNU 1422

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0.38 UTI
0.3
CN
0.86
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.86 Dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1422 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction 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 – 62.824 51.232 0.331 -0.391 -0.663 –
Hunt & Reffert 2024 62.839 51.217 0.324 -0.39 -0.66 –
Cavallo et al. 2024 62.848 51.254 0.329 – – –
Hunt & Reffert 2023 62.839 51.217 0.324 -0.39 -0.66 –
He et al. 2023 62.834 51.236 0.349 -0.383 -0.664 –

💡 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 – – – – – 333* – –
Cavallo et al. 2024 3.42 2.85 – 59 0.560 – – –
Hunt & Reffert 2023 2.80 2.93 1.32 62 – – – –
He et al. 2023 2.51 2.95 – 398 – – – –

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

Visualization

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