CWNU 1769

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0.47 UTI
0.32
CN
0.88
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.88 Dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1769 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (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 – 120.106 -32.27 0.453 -2.732 3.059 –
Hunt & Reffert 2024 120.137 -32.246 0.469 -2.737 3.092 –
Cavallo et al. 2024 120.113 -32.256 0.471 – – –
Hunt & Reffert 2023 120.137 -32.246 0.469 -2.737 3.092 –
He et al. 2023 120.139 -32.248 0.46 -2.73 3.062 –

💡 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 – – – – – 85* – –
Cavallo et al. 2024 1.90 1.91 – 37 -0.360 – – –
Hunt & Reffert 2023 1.99 1.63 0.32 157 – – – –
He et al. 2023 2.04 2.00 – 63 – – – –

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

Visualization

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