activity
19932023
most citedCompetitive accretion in embedded stellar cluster

606 citations · 12.5k across the 161 of their papers we have counts for

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Showing 2009Show all

6 papers · 1 filter

astro-ph.GA2009★ 18 cited

The physics and modes of star cluster formation: simulations

Cathie Clarke

We review progress in numerical simulations of star cluster formation. These simulations involve the bottom-up assembly of clusters through hierarchical mergers, which produces a f…

astro-ph.EP2009★ 132 cited

Metallicity, planet formation, and disc lifetimes

Barbara Ercolano, Cathie Clarke

The formation of planets within a disc must operate within the time frame of disc dispersal, it is thus crucial to establish what is the dominant process that disperses the gaseous…

astro-ph.GA2009★ 82 cited

The effects of opacity on gravitational stability in protoplanetary discs

Peter Cossins, Giuseppe Lodato, Cathie Clarke

In this paper we consider the effects of opacity regimes on the stability of self-gravitating protoplanetary discs to fragmentation into bound objects. Using a self-consistent 1-D…

astro-ph.SR2009★ 370 cited

Radiation-Hydrodynamic Models of X-Ray & EUV Photoevaporating Protoplanetary Discs

J. E. Owen, B. Ercolano, C. J. Clarke +1

(Abridged) We present the first radiation-hydrodynamic model of a protoplanetary disc irradiated with an X-EUV spectrum. In a model where the total ionizing luminosity is divided e…

astro-ph.SR2009★ 219 cited

Pseudo-viscous modeling of self-gravitating discs and the formation of low mass ratio binaries

C. Clarke

We present analytic models for the local structure of self-regulated self-gravit ating accretion discs that are subject to realistic cooling. Such an approach can be used to predic…

astro-ph.SR2009★ 52 cited

The transition disc frequency in M stars

Barbara Ercolano, Cathie J. Clarke, Thomas P. Robitaille

We re-examine the recent suggestion of a high fraction of transition discs (i.e. those with a cleared inner hole) in M stars, motivated by the fact that we expect that, for M stars…