CWNU 2269

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0.42 UTI
0.5
CN
0.36
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.36 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2269 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Relatively close 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 – 185.154 -61.695 0.291 -5.785 -0.068 -38.179
Hunt & Reffert 2024 185.136 -61.684 0.289 -5.774 -0.094 -38.152
Cavallo et al. 2024 185.119 -61.697 0.291 – – –
Hunt & Reffert 2023 185.136 -61.684 0.289 -5.774 -0.094 -38.152
He et al. 2023 185.152 -61.692 0.301 -5.823 -0.068 -38.18

💡 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 – – – – – 471* – –
Cavallo et al. 2024 2.30 1.38 – 219 -0.260 – – –
Hunt & Reffert 2023 3.06 1.59 0.71 29 – – – –
He et al. 2023 2.82 1.80 – 25 – – – –

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

Visualization

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