Deriving the intrinsic properties of M51 with radiative transfer models

ABSTRACT A quantitative derivation of the intrinsic properties of galaxies related to their fundamental building blocks, gas, dust, and stars is essential for our understanding of galaxy evolution. A fully self-consistent derivation of these properties can be achieved with radiative transfer (RT) me...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2023-09, Vol.526 (1), p.118-137
Hauptverfasser:	Inman, Christopher J, Popescu, Cristina C, Rushton, Mark T, Murphy, David
Format:	Artikel
Sprache:	eng
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