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
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
10 September 2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 481, Heft: 2, Pages: 2507-2522 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2415 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2415 Verlag, Volltext: https://academic.oup.com/mnras/article/481/2/2507/5094585 
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| Verfasserangaben: | Stefan Reissl, Amelia M. Stutz, Robert Brauer, Eric W. Pellegrini, Dominik R.G. Schleicher and Ralf S. Klessen |
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| 520 | |a 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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