CWNU 1804

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0.48 UTI
0.28
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1804 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.
Distant High extinction Metal-rich Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 53.071 55.034 0.325 -0.878 -0.77 –
Hunt & Reffert 2024 53.059 55.032 0.329 -0.855 -0.794 –
Cavallo et al. 2024 53.095 55.045 0.326 – – –
Hunt & Reffert 2023 53.059 55.032 0.329 -0.855 -0.794 –
He et al. 2023 53.068 55.034 0.326 -0.839 -0.796 –

💡 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 – – – – – 337* – –
Cavallo et al. 2024 3.77 3.73 – 37 0.760 – – –
Hunt & Reffert 2023 2.92 4.41 2.03 36 – – – –
He et al. 2023 3.24 4.90 – 4 – – – –

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

Visualization

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