activity
20142023
most citedMagnetically controlled mass loss from extrasolar planets in close orbits

139 citations · 254 across the 10 of their papers we have counts for

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Showing astro-ph.SRShow all

5 papers · 1 filter

astro-ph.SR201621 cited

Dust traps as planetary birthsites: basics and vortex formation

James E. Owen, Juna A. Kollmeier

We present a simple model for low-mass planet formation and subsequent evolution within "transition" discs. We demonstrate quantitatively that the predicted and observed structure…

astro-ph.SR20149 cited

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-ph.SR201420 cited

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…

astro-ph.SR20146 cited

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…

astro-ph.SR201429 cited

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…