activity
20162020
most citedMagnetized filamentary gas flows feeding the young embedded cluster in Serpens South

89 citations · 152 across the 5 of their papers we have counts for

collaborators

16 papers

astro-ph.GA202089 cited

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…

astro-ph.GA2020

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…

astro-ph.GA2020

Synthetic observations of deuterated molecules in massive prestellar cores

Joaquin Zamponi F., Andrea Giannetti, Stefano Bovino +5

Young massive stars are usually found embedded in dense massive molecular clumps and are known for being highly obscured and distant. During their formation process, deuteration is…

astro-ph.GA2020

Synthetic observations of spiral arm tracers of a simulated Milky Way analog

Stefan Reissl, Jeroen M. Stil, En Chen +16

Context: The Faraday rotation measure (RM) is often used to study the magnetic field strength and orientation within the ionized medium of the Milky Way. Observations indicate a RM…

astro-ph.GA202016 cited

Less than the sum of its parts: the dust-corrected H luminosity of star-forming galaxies explored at different spatial resolutions with MaNGA and MUSE

N. Vale Asari, V. Wild, A. L. de Amorim +10

The H and H emission line luminosities measured in a single integrated spectrum are affected in non-trivial ways by point-to-point variations in dust attenuation in a galaxy.…

astro-ph.SR20209 cited

Linear dust polarization during the embedded phase of protostar formation

M. Kuffmeier, S. Reissl, S. Wolf +2

Measuring polarization from thermal dust emission can provide constraints on the magnetic field structure around embedded protostars. However, interpreting the observations is chal…