CWNU 2004

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0.32 UTI
0.31
CN
0.29
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 0.29 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2004 is a poorly populated, loose object of intermediate 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.
Distant 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 – 15.321 63.116 0.231 -1.47 -0.172 -30.062
Hunt & Reffert 2024 15.268 63.114 0.221 -1.464 -0.186 –
Cavallo et al. 2024 15.294 63.095 0.223 – – –
Hunt & Reffert 2023 15.268 63.114 0.221 -1.464 -0.186 –
He et al. 2023 15.454 63.137 0.298 -1.483 -0.119 -30.06

💡 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 – – – – – 585* – –
Cavallo et al. 2024 4.25 2.51 – 23 0.400 – – –
Hunt & Reffert 2023 4.01 2.62 2.12 41 – – – –
He et al. 2023 2.88 2.30 – 398 – – – –

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

Visualization

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