Determination of Planetary Nebulae angular diameters from radio continuum spectral energy distribution modelling

@inproceedings{Bojii2021DeterminationOP,
  title={Determination of Planetary Nebulae angular diameters from radio continuum spectral energy distribution modelling},
  author={I S Boji{\vc}i{\'c} and Miroslav D. Filipovi{\'c} and Dejan Uro{\vs}evi{\'c} and Quentin A. Parker and T. J. Galvin},
  year={2021}
}
Powerful new, high resolution, high sensitivity, multi-frequency, wide-field radio surveys such as the Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) are emerging. They will offer fresh opportunities to undertake new determinations of useful parameters for various kinds of extended astrophysical phenomena. Here, we consider specific application to angular size determinations of Planetary Nebulae (PNe) via a new radio continuum Spectral Energy… 

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