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Magnetized filamentary gas flows feeding the young embedded cluster in Serpens South
Thushara G. S. Pillai, Dan P. Clemens, Stefan Reissl +11
Observations indicate that molecular clouds are strongly magnetized, and that magnetic fields influence the formation of stars. A key observation supporting the conclusion that mol…
The impact of episodic outflow feedback on stellar multiplicity and the star formation efficiency
P. F. Rohde, S. Walch, S. D. Clarke +3
The accretion of material onto young protostars is accompanied by the launching of outflows. Observations show that accretion, and therefore also outflows, are episodic. However, t…
Magnetic fields in star-forming systems (II): examining dust polarization, the Zeeman effect, and the Faraday rotation measure as magnetic field tracers
Stefan Reissl, Amelia M. Stutz, Ralf S. Klessen +2
The degree to which the formation and evolution of clouds and filaments in the interstellar medium is regulated by magnetic fields remains an open question. Yet the fundamental pro…
From parallel to perpendicular -- On the orientation of magnetic fields in molecular clouds
D. Seifried, S. Walch, M. Weis +4
We present synthetic dust polarization maps of simulated molecular clouds (MCs) with the goal to systematically explore the origin of the relative orientation of the magnetic field…