This article has been accepted for publication in MNRAS ©: 2016: The authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.We acknowledge the comments received from an anonymous referee, which helped to improve the quality of this paper. GALC acknowledges the support of an STFC PhD studentship. This research utilised Queen Mary’s MidPlus computational facilities, supported by QMUL Research-IT and funded by EPSRC grant EP/K000128/
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The Solar System, together with some exoplanetary systems, is known to host multiple planets. These ...
Some observed exoplanets cannot be explained in the standard core accretion paradigm. An alternative...
The discovery of giant planets in wide orbits represents a major challenge for planet formation theo...
Aims: The connection between initial disc conditions and final orbital and physical properties of pl...
GALC acknowledges the support of an STFC PhD studentship. The simulations presented in this paper we...
PhDI examine the effects on planetary system formation of radiatively inefficient disc models where...
PhDThe diversity in observed planets and planetary systems has raised the question of whether they c...
In order to explain the main characteristics of the observed population of extrasolar planets and th...
We know now that discs of gas and dust, so-called protoplanetary discs, form planets as side-product...
We use high-resolution three-dimensional smoothed particle hydrodynamic (SPH) simulations to study t...
The Earth is not the only planet in the universe. It has been known for millennia that there are oth...
© 2018, The Author(s). Planets form in circumstellar discs around young stars. Starting with sub-mic...
Numerical simulations show that the migration of growing planetary cores may be dominated by turbule...
The existence of giant planets on wide orbits ($\stackrel{>}{_\sim}100$AU) challenge planet formatio...
To estimate the occurrence of terrestrial exoplanets and maximize the chance of finding them, it is ...
The Solar System, together with some exoplanetary systems, is known to host multiple planets. These ...
Some observed exoplanets cannot be explained in the standard core accretion paradigm. An alternative...
The discovery of giant planets in wide orbits represents a major challenge for planet formation theo...