Polarised emission from aligned dust grains in nearby galaxies : predictions from the Auriga simulations

Context. Polarised emission from non-spherical dust grains contains information about the alignment of these dust grains and traces the structure of the interstellar magnetic field. Methods: We post-processed a set of Milky-Way-like galaxies from the Auriga project, assuming a dust mix consisting of...

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Bibliographische Detailangaben

Hauptverfasser:	Vandenbroucke, Bert, Baes, Maarten, Camps, Peter, Kapoor, Anand Utsav, Barrientos Acevedo, Daniela, Bernard, J.-P
Format:	Artikel
Sprache:	eng
Schlagworte:	ALIGNMENT DISC GALAXIES galaxies IMAGING POLARIMETRY magnetic fields MAGNETIC-FIELD methods numerical Physics and Astronomy polarization radiative transfer RADIATIVE-TRANSFER CODE RESOLUTION STATISTICS SUPERNOVA-REGULATED ISM
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