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20062023
most citedPhotoevaporation of protoplanetary discs II: evolutionary models and observable properties

478 citations · 3.5k across the 54 of their papers we have counts for

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7 papers · 1 filter

astro-ph2008★ 1 cited

Gas Evolution in Protoplanetary Disks

Peter Woitke, Bill Dent, Wing-Fai Thi +9

This article summarizes a Splinter Session at the Cool Stars XV conference in St. Andrews with 3 review and 4 contributed talks. The speakers have discussed various approaches to u…

astro-ph2007★ 57 cited

From discs to planetesimals I: evolution of gas and dust discs

Richard Alexander

I review the processes that shape the evolution of protoplanetary discs around young, solar-mass stars. I first discuss observations of protoplanetary discs, and note in particular…

astro-ph2007★ 50 cited

The Monitor project: JW 380 -- a 0.26, 0.15 Msol pre main sequence eclipsing binary in the Orion Nebula Cluster

Jonathan Irwin, Suzanne Aigrain, Simon Hodgkin +14

We report the discovery of a low-mass (0.26 +/- 0.02, 0.15 +/- 0.01 Msol) pre-main-sequence eclipsing binary with a 5.3 day orbital period. JW 380 was detected as part of a high-ca…

astro-ph2006★ 59 cited

Constraints on the Stellar Mass Function from Stellar Dynamics at the Galactic Center

R. D. Alexander, M. C. Begelman, P. J. Armitage

We consider the dynamical evolution of a disk of stars orbiting a central black hole. In particular, we focus on the effect of the stellar mass function on the evolution of the dis…

astro-ph2006★ 478 cited

Photoevaporation of protoplanetary discs II: evolutionary models and observable properties

R. D. Alexander, C. J. Clarke, J. E. Pringle

We present a new model for protoplanetary disc evolution. This model combines viscous evolution with photoevaporation of the disc, in a manner similar to Clarke, Gendrin & Sotomayo…

astro-ph2006★ 296 cited

Photoevaporation of protoplanetary discs I: hydrodynamic models

R. D. Alexander, C. J. Clarke, J. E. Pringle

In this paper we consider the effect of the direct ionizing stellar radiation field on the evolution of protoplanetary discs subject to photoevaporative winds. We suggest that mode…