CWNU 1446

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0.59 UTI
0.43
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1446 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Metal-poor 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 – 271.896 -25.107 0.675 0.803 -1.512 –
Hunt & Reffert 2024 271.89 -25.119 0.659 0.806 -1.515 –
Cavallo et al. 2024 271.896 -25.112 0.658 – – –
Hunt & Reffert 2023 271.89 -25.119 0.659 0.806 -1.515 –
He et al. 2023 271.893 -25.113 0.675 0.81 -1.51 –

💡 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 – – – – – 230* – –
Cavallo et al. 2024 1.13 2.94 – 18 -0.890 – – –
Hunt & Reffert 2023 1.41 1.96 1.95 65 – – – –
He et al. 2023 1.41 2.30 – 25 – – – –

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

Visualization

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