Dr. Constantina M. Fotopoulou | Astrophysicist

About me

I am a postdoctoral researcher at the Theoretical Astrophysics Group Cologne (TAC), working within the DFG Collaborative Research Centre Habitats of Massive Stars Across Cosmic Time (SFB 1601), specializing in computational astrophysics. My research focuses on the turbulent, multi-phase interstellar medium (ISM), investigating its physical and chemical properties and its role in star formation and galaxy evolution. I approach these questions using high-resolution numerical simulations and synthetic observations, aiming to bridge theoretical models with observational data.

I grew up in Athens, Greece where I studied Physics at the National and Kapodistrian University of Athens (NKUA) and obtained my MSc in Astrophysics at the same institution. Fascinated by the physical processes and mechanisms that underlie galaxy formation and evolution combined with a genuine passion for coding, I ventured to Germany, where I earned my PhD in Astronomy from the Max Planck Institute of Astrophysics (MPA) and the Ludwig Maximilian University of Munich (LMU).

As a scientist, I strive to contribute to the advancement of knowledge and the pursuit of innovative applications, while bridging the gap between fundamental research and technological development. Beyond research, I am actively involved in volunteering and public outreach initiatives, working to make science accessible to diverse audiences and to inspire engagement and inclusivity in STEM.

Have a look at my CV or read more about my research.

“The nitrogen in our DNA, the calcium in our teeth, the iron in our blood, the carbon in our apple pies were made in the interiors of collapsing stars. We are made of starstuff.”
― Carl Sagan, Cosmos

My Research in Extragalactic Astrophysics

My research focuses on galaxy evolution, through the study of the turbulent multi-phase interstellar medium (ISM), star formation, and feedback mechanisms across diverse galactic environments, through a combination of observational and numerical approaches.

As part of the GRIFFIN project, I used a high-resolution hydrodynamic simulation to study starburst-driven outflows and the lifecycle of cold star-forming clouds in a low-metallicity dwarf galaxy merger (Fotopoulou et al., 2024). Our analysis revealed that the starburst impacts the ISM by forming short-lived cold clouds with realistic mass and size distributions, in good agreement with observations (e.g. Larson relations) and validates our model’s ability to simulate star-forming clouds and feedback processes in low-metallicity environments.

Zoom sequence of the gas distribution colour-coded by the mass weighted temperature. — Zoom sequence of the gas distribution colour-coded by the mass weighted temperature (first three panels) of the GRIFFIN simulation at 300 Myr (right panel) from 10 kpc down to 100 pc. In the bottom right panel, we show a zoom on to a massive cloud with its environment. The raw particle distribution of the cloud is shown in the bottom left panel. Fotopoulou et al. (2024)

Using ALMA CO observations of the galaxy 4C12.50 (Fotopoulou et al., 2019), I studied the structure and dynamics, of its molecular gas. Our findings reveal high-velocity outflow components driven by AGN jets assisted by starburst activity, highlighting the impact of feedback on the ISM and its interplay with star formation.