activity
20012007
most citedA comparative study of disc-planet interaction

446 citations · 837 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph2007★ 53 cited

Multiplicity Among Young Brown Dwarfs and Very Low Mass Stars

Mirza Ahmic, Ray Jayawardhana, Alexis Brandeker +4

Characterizing multiplicity in the very low mass (VLM) domain is a topic of much current interest and fundamental importance. Here we report on a near-IR AO imaging survey of 31 yo…

astro-ph2006★ 446 cited

A comparative study of disc-planet interaction

M. de Val-Borro, R. G. Edgar, P. Artymowicz +20

We perform numerical simulations of a disc-planet system using various grid-based and smoothed particle hydrodynamics (SPH) codes. The tests are run for a simple setup where Jupite…

astro-ph2006★ 3 cited

New observational frontiers in the multiplicity of young stars

G. Duchene, E. Delgado-Donate, K. Haisch +2

It has now been known for over a decade that low-mass stars located in star-forming regions are very frequently members of binary and multiple systems, even more so than main seque…

astro-ph2005★ 49 cited

Constraints on the formation mechanism of the planetary mass companion of 2MASS 1207334-393254

G. Lodato, E. Delgado-Donate, C. J. Clarke

In this paper we discuss the nature and the possible formation scenarios of the companion of the brown dwarf 2MASS 1207334-393254. We initially discuss the basic physical propertie…

astro-ph2004★ 119 cited

On the properties of young multiple stars

E. J. Delgado-Donate, C. J. Clarke, M. R. Bate +1

Abridged/ We present numerical results on the properties of young binary and multiple stellar systems. Our analysis is based on a series of SPH + Nbody simulations of the fragmenta…

astro-ph2003★ 71 cited

The dependence of the sub-stellar IMF on the initial conditions for star formation

E. J Delgado-Donate, C. J. Clarke, M. R. Bate

Abridged: We have undertaken a series of hydrodynamical simulations of multiple star formation in small turbulent molecular clouds. Our goal is to determine the sensitivity of the…