CWNU 204

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0.33 UTI
0.0
CN
0.63
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.63 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 204 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 121.073 -29.218 0.569 -3.701 2.84 56.587
Hunt & Reffert 2024 121.071 -29.215 0.563 -3.686 2.842 35.928
Cavallo et al. 2024 121.045 -29.219 0.56 – – –
Hunt & Reffert 2023 121.071 -29.215 0.563 -3.686 2.842 35.928
He et al. 2022 121.067 -29.212 0.55 -3.69 2.9 –

💡 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 – – – – – 128* – –
Cavallo et al. 2024 1.79 0.60 – 204 0.340 – – –
Hunt & Reffert 2023 1.63 0.32 0.78 398 – – – –
He et al. 2022 1.35 0.36 – 40 0.051 – – –

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

Visualization

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