Status: unreviewed
revisit date: None
Application status: none
LOR status: not_needed
Department(s)/lab(s):
Physics | Astrophysics Group @ Imperial
Summary:
Owen works on the theory and observational consequences of protoplanetary disk evolution, photoevaporation and exoplanet demographics, explaining features such as the observed radius gap in close-in exoplanets.
Created at: July 8, 2026, 8:39 p.m.
Updated at: July 8, 2026, 8:39 p.m.
Metadata: Imperial Physics Astrophysics Group profile, reviewed Jul 2026.