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Modelling Local Bubble analogs: synthetic dust polarization maps
E Maconi, J D Soler, S Reissl, P Girichidis, R S Klessen, P Hennebelle, S Molinari, L Testi, R J Smith, M C Sormani, J W Teh and A Traficante Monthly Notices of the Royal Astronomical Society 523(4) 5995 (2023) https://doi.org/10.1093/mnras/stad1854
Time-dependent Monte Carlo continuum radiative transfer
Radiative transfer simulations for in-situ particle size diagnostic in reactive, particle growing plasmas
Julia Kobus, Andreas Petersen, Franko Greiner and Sebastian Wolf Journal of Physics D: Applied Physics 55(35) 355202 (2022) https://doi.org/10.1088/1361-6463/ac74f6
Recent progress with observations and models to characterize the magnetic fields from star-forming cores to protostellar disks
Long Baseline Observations of the HD 100546 Protoplanetary Disk with ALMA
Sebastián Pérez, Simon Casassus, Antonio Hales, Sebastián Marino, Anthony Cheetham, Alice Zurlo, Lucas Cieza, Ruobing Dong, Felipe Alarcón, Pablo Benítez-Llambay, Ed Fomalont and Henning Avenhaus The Astrophysical Journal Letters 889(1) L24 (2020) https://doi.org/10.3847/2041-8213/ab6b2b
Unbiased Monte Carlo continuum radiative transfer in optically thick regions
Gas Density Perturbations Induced by One or More Forming Planets in the AS 209 Protoplanetary Disk as Seen with ALMA
Cécile Favre, Davide Fedele, Luke Maud, Richard Booth, Marco Tazzari, Anna Miotello, Leonardo Testi, Dmitry Semenov and Simon Bruderer The Astrophysical Journal 871(1) 107 (2019) https://doi.org/10.3847/1538-4357/aaf80c
Radiative Transfer with POLARIS. II. Modeling of Synthetic Galactic Synchrotron Observations
G H-M Bertrang, H Avenhaus, S Casassus, et al. Monthly Notices of the Royal Astronomical Society 474(4) 5105 (2018) https://doi.org/10.1093/mnras/stx3052
Observability of planet–disc interactions in CO kinematics
Sebastián Pérez, S Casassus and P Benítez-Llambay Monthly Notices of the Royal Astronomical Society: Letters 480(1) L12 (2018) https://doi.org/10.1093/mnrasl/sly109
Constraints on observing brightness asymmetries in protoplanetary disks at solar system scale