Dr. Florian Kirchschlager


Postdoctoral researcher


Ghent University




About

I am a computational astrophysicist studying dust in supernova remnants and in the interstellar medium. As a postdoc in the Department of Physics & Astronomy at Ghent University , I investigate the transport, destruction and growth of dust in a moving gas. In the past, I also worked on dust in circumstellar discs and on optical properties of non-spherical dust grains.

My research

The focus of my research is the evolution of dust in the presence of shocks occuring at supernovae explosions. Dust grains in the clumpy ejecta of supernova remnants have to pass the reverse shock before they can be ejected into the ISM, while ISM dust is processed by the forward shock blast wave of the supernova. In this context, I have developed the dust-processing code Paperboats (Kirchschlager et al. 2019, 2023) which allows to investigate the dust transport, dust destruction by sputtering, vaporization or fragmentation, and dust growth via coagulation, gas accretion or ion trapping. Furthermore, I am involved in observations done with telescopes like the James Webb Space Telescope (JWST) and the Very Large Telescope (VLT).

In the last couple of years, I have also worked on both observational and theoretical projects in the field of protoplanetary and debris discs using near- and mid-infrared observations and 3D radiative transfer simulations. In particular, I am an observer and modeller of hot exozodiacal dust around main-sequence stars. Beyond that I studied for several years the influence of dust properties like grain porosity and grain shape on the intensity and polarisation of circumstellar discs.

Recent highlights

Spring 2026: I am pleased to announce that I have been awarded a DFG Heisenberg grant and will start my new position at University of Hamburg in September.


30.11.2025: My PhD student T. Scheffler has just published his paper on dust destruction by supernova forward shocks propagating through a turbulent interstellar medium. The study quantifies how ISM turbulence affects dust survival and destruction efficiencies, with important implications for dust evolution in galaxies. Reference: Scheffler, Sartorio, Kirchschlager et al. (2026)



Upcoming events

  • Onganiser of the symposium "Supernovae and their remnants: from stellar death to galactic evolution", at the European Astronomical Society Annual Meeting (EAS), 29 June - 3 July 2026, Lausanne, Switzerland