Star and planet formation

I use hydrodynamical, radiative transfer and chemical models to develop our understanding of how stars and planets form and of protoplanetary disc structures.
I completed my PhD exploring the observational characteristics of the first hydrostatic core in 2019 at the University of Exeter, UK and currently work at the Royal Observatory, Edinburgh, UK. You can find my PhD thesis here.
Follow this link to view my publications in ADS.