CWNU 39

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0.33 UTI
0.28
CN
0.36
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.0 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 0.36 Loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 39 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied 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 – 92.682 23.343 0.515 -0.321 -1.764 –
Zhang et al. 2024 92.74 23.434 – – – –
Hunt & Reffert 2024 92.74 23.434 0.51 -0.317 -1.763 –
Cavallo et al. 2024 92.666 23.384 0.509 – – –
Hunt & Reffert 2023 92.74 23.434 0.51 -0.317 -1.763 –
He et al. 2022 92.633 23.346 0.51 -0.32 -1.76 –

💡 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
Zhang et al. 2024 – – – – -0.261* – – –
Hunt & Reffert 2024 – – – – – 237* – –
Cavallo et al. 2024 1.95 1.19 – 26 -0.150 – – –
Hunt & Reffert 2023 1.87 1.12 1.42 81 – – – –
He et al. 2022 1.91 1.44 – 32 -0.642 – – –

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

Visualization

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