139 citations · 203 across the 6 of their papers we have counts for
6 papers
Probing X-ray photoevaporative winds through their interaction with ionising radiation in cluster environments: the case for X-ray proplyds
C. J. Clarke, James. E. Owen
We show that if young low mass stars undergo vigorous X-ray driven disc winds, these may be detected in clusters through their interaction with ionising radiation from massive star…
Astro & cosmo-chemical consequences of accretion bursts I: the D/H ratio of water
James E. Owen, Emmanuel Jacquet
The D/H ratio of water in protostellar systems is a result of both inheritance from the parent molecular cloud and isotopic exchange in the disc. A possibly widespread feature of d…
Magnetically Controlled Outflows from Planets
Fred C. Adams, James E. Owen
Hot Jupiters can experience mass loss driven by heating from UV radiation from their host stars, and this flow is often controlled by magnetic fields. More specifically, near the p…
Importance of thermal diffusion in the gravo-magnetic limit cycle
James E. Owen, Philip J. Armitage
We consider the role of thermal diffusion due to turbulence and radiation on accretion bursts that occur in protoplanetary discs which contain dead zones. Using 1D viscous disc mod…
Magnetically controlled mass loss from extrasolar planets in close orbits
James E. Owen, Fred C. Adams
We consider the role magnetic fields play in guiding and controlling mass-loss via evaporative outflows from exoplanets that experience UV irradiation. First we present analytic re…
Snow-lines as probes of turbulent diffusion in protoplanetary discs
James E. Owen
Sharp chemical discontinuities can occur in protoplanetary discs, particularly at `snow-lines' where a gas-phase species freezes out to form ice grains. Such sharp discontinuities…