CWNU 2016

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0.32 UTI
0.27
CN
0.48
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.48 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2016 is a poorly populated, loose object of low 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 – 111.352 -8.063 0.483 -2.871 2.579 –
Hunt & Reffert 2024 111.289 -8.041 0.46 -2.878 2.581 –
Cavallo et al. 2024 111.393 -8.036 0.463 – – –
Hunt & Reffert 2023 111.289 -8.041 0.46 -2.878 2.581 –
He et al. 2023 111.319 -8.071 0.488 -2.842 2.579 –

💡 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 – – – – – 100* – –
Cavallo et al. 2024 1.86 0.45 – 178 -0.200 – – –
Hunt & Reffert 2023 1.97 0.09 0.64 157 – – – –
He et al. 2023 2.09 0.10 – 501 – – – –

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

Visualization

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