33 citations · 64 across the 2 of their papers we have counts for
7 papers
Spatial distribution of the aromatic and aliphatic carbonaceous nano-grain features in the protoplanetary disk around HD 100546
Emilie Habart, Thomas Boutéraon, Robert Brauer +4
Carbonaceous nano-grains are present at the surface of protoplanetary disks around Herbig Ae/Be stars, where most of the central star UV energy is dissipated. Efficiently coupled t…
A systematic study of radiative torque grain alignment in the diffuse interstellar medium
Stefan Reissl, Vincent Guillet, Robert Brauer +3
Context. Planck observations demonstrated that the grain alignment efficiency is almost constant in the diffuse ISM. Aims. We test if the Radiative Torque (RAT) theory is compatibl…
Radiative transfer with POLARIS. II.: Modeling of synthetic Galactic synchrotron observations
Stefan Reissl, Robert Brauer, Ralf S. Klessen +1
We present an updated version of POLARIS, a well established code designated for dust polarisation and line radiative transfer (RT) in arbitrary astrophysical environments. We exte…
Indirect evidence of significant grain growth in young protostellar envelopes from polarized dust emission
Valeska Valdivia, Anaelle Maury, Robert Brauer +4
How and when in the star formation sequence do dust grains start to grow into pebbles is a cornerstone question to both star and planet formation. We compute the polarized radiativ…
Magnetic fields in star forming systems (I): Idealized synthetic signatures of dust polarization and Zeeman splitting in filaments
Stefan Reissl, Amelia M. Stutz, Robert Brauer +3
We use the POLARIS radiative transport code to generate predictions of the two main observables directly sensitive to the magnetic field morphology and strength in filaments: dust…
Magnetic fields in circumstellar disks: The potential of Zeeman observations
R. Brauer, S. Wolf, M. Flock
Context. Recent high angular resolution polarimetric continuum observations of circumstellar disks provide new insights into their magnetic field. However, direct constraints are l…