Thiébaut-Antoine Schirmer
Cosmic dust plays a crucial role in the physico-chemistry of the Universe. The dust properties (i.e. composition, size, and shape) are however still not well understood. In addition, the wide disparity in physical conditions (i.e. irradiation and density) across the Universe triggers an evolution of the dust properties through phenomena such as accretion, coagulation, destruction. My main objective is to understand how dust evolves as a response to the physical conditions and to constrain its properties.
Based on observations from the infrared to the millimeter range, I study dust properties in various environments, from their creation in the atmosphere of evolved stars (AGBs) to the early universe in highredshift galaxies, through extreme environments nearby AGNs.
Showing 12 publications
OH as a probe of the warm-water cycle in planet-forming disks
PDRs4All V. Modelling the dust evolution across the illuminated edge of the Orion Bar
A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk
PDRs4All: III. JWST's NIR spectroscopic view of the Orion Bar
High-angular-resolution NIR view of the Orion Bar revealed by Keck/NIRC2
Editorial: Cosmic dust—its formation, processing, and destruction
The extremely sharp transition between molecular and ionized gas in the Horsehead nebula
The Origin of Dust Polarization in the Orion Bar
Formation of the methyl cation by photochemistry in a protoplanetary disk
Nano-grain depletion in photon-dominated regions
PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars
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