Magnetic fields in star-forming systems (I): idealized synthetic signatures of dust polarization and Zeeman splitting in filaments

ABSTRACT. We use the polaris radiative transfer code to generate predictions of the two main observables directly sensitive to the magnetic field morphology an

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Bibliographic Details
Main Authors:	Reißl, Stefan (Author) , Pellegrini, Eric William (Author) , Klessen, Ralf S. (Author)
Format:	Article (Journal)
Language:	English
Published:	10 September 2018
In:	Monthly notices of the Royal Astronomical Society Year: 2018, Volume: 481, Issue: 2, Pages: 2507-2522
ISSN:	1365-2966
DOI:	10.1093/mnras/sty2415
Online Access:	Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2415 Verlag, Volltext: https://academic.oup.com/mnras/article/481/2/2507/5094585
Author Notes:	Stefan Reissl, Amelia M. Stutz, Robert Brauer, Eric W. Pellegrini, Dominik R.G. Schleicher and Ralf S. Klessen

Description
Summary:	ABSTRACT. We use the polaris radiative transfer code to generate predictions of the two main observables directly sensitive to the magnetic field morphology an
Item Description:	Gesehen am 11.12.2019
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/sty2415