CWNU 326

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0.49 UTI
0.45
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 326 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 moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate 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 – 298.52 29.109 0.468 -0.622 -2.556 -12.305
Hunt & Reffert 2024 298.533 29.115 0.459 -0.649 -2.577 -0.015
Cavallo et al. 2024 298.528 29.112 0.463 – – –
Hunt & Reffert 2023 298.533 29.115 0.459 -0.649 -2.577 -0.015
He et al. 2022 298.523 29.122 0.47 -0.6 -2.55 4.4

💡 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 – – – – – 169* – –
Cavallo et al. 2024 2.10 1.39 – 490 0.690 – – –
Hunt & Reffert 2023 2.05 1.80 0.76 255 – – – –
He et al. 2022 1.51 1.62 – 1000 -0.930 – – –

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

Visualization

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