CWNU 2266

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0.58 UTI
0.66
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.66 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2266 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close High extinction Massive 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 – 247.065 -51.097 0.336 -0.816 -2.455 -43.409
Hunt & Reffert 2024 247.061 -51.092 0.331 -0.809 -2.464 -43.412
Cavallo et al. 2024 247.057 -51.104 0.333 – – –
Hunt & Reffert 2023 247.061 -51.092 0.331 -0.809 -2.464 -43.412
He et al. 2023 247.062 -51.134 0.348 -0.816 -2.447 -46.29

💡 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 – – – – – 1168* – –
Cavallo et al. 2024 2.75 3.77 – 166 0.370 – – –
Hunt & Reffert 2023 2.65 3.63 2.69 87 – – – –
He et al. 2023 2.51 3.90 – 100 – – – –

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

Visualization

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