Timmy N. Delage
Imperial College London, Chalmers University of Technology, Max Planck Institute for Astronomy
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Stellar, planetary, and galactic studies · Astro and Planetary Science · Astrophysics and Star Formation Studies
About
I am a Royal Society Career Development Fellow in the Astrophysics Group of Imperial College London. I combine theoretical modelling and computer simulations to build a coherent picture of how gas and dust evolve and interact in planet-forming environments, ultimately giving rise to planets. By comparing model predictions with observations of planet-forming environments and extra-solar planets, I aim to develop a predictive theory of planet formation and help interpret what we observe with telescopes.
My expertise lies in modelling the complex interplay between dust microphysics, gas ionisation and magnetic processes, and how these processes shape the long-term evolution of planet-forming environments. I have developed a unique numerical framework for these environments that couples the long-term evolution of their gas and dust content, including dust growth and dynamics, with nonideal magnetohydrodynamic calculations. I use this framework to understand how, when and where the building blocks of planets form.
Employment
-
Imperial College London Royal Society Career Development Fellow2024 - Present
-
Chalmers University of Technology Independent Chalmers Initiative on Cosmic Origins Postdoctoral Fellow2023 - 2024
Education
-
Max Planck Institute for Astronomy PhD in Astrophysics2019 - 2023
Projects & Funding
-
Royal Society Career Development Fellowship 2024 Royal Society2024 - Present
-
Independent Chalmers Initiative on Cosmic Origins Fellowship 2023 Chalmers University of Technology2023 - 2024
Publications (9)
- Evolution of Dust In Protoplanetary Disks With Magnetized Winds Save
- The impact of dust evolution on the dead zone outer edge in magnetized protoplanetary disks Save
- EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates of Planets around Late-M Dwarfs within 15 pc Save
- EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates for Late M Dwarfs within 15 pc Save
- Explaining transition disks without massive planets Save
- Steady-state accretion in magnetized protoplanetary disks Save
- Large gaps and high accretion rates in photoevaporative transition disks with a dead zone Save
- Constraining the properties of the potential embedded planets in the disk around HD 100546 Save
- Large gaps and high accretion rates in photoevaporative transition disks with a dead zone Save