CWNU 2265

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0.27 UTI
0.0
CN
0.1
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2265 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported 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 – 167.709 -57.892 0.29 -6.421 2.134 5.275
Hunt & Reffert 2024 167.697 -57.887 0.289 -6.419 2.122 –
Cavallo et al. 2024 167.735 -57.896 0.288 – – –
Hunt & Reffert 2023 167.697 -57.887 0.289 -6.419 2.122 –
He et al. 2023 167.726 -57.915 0.295 -6.413 2.127 26.74

💡 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 – – – – – 252* – –
Cavallo et al. 2024 2.41 0.62 – 309 -0.010 – – –
Hunt & Reffert 2023 3.04 1.05 1.02 94 – – – –
He et al. 2023 2.88 0.75 – 794 – – – –

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

Visualization

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