88 citations · 178 across the 9 of their papers we have counts for
9 papers
Stable habitable zones of single Jovian planet systems
Matthew T. Agnew, Sarah T. Maddison, Elodie Thilliez +1
With continued improvement in telescope sensitivity and observational techniques, the search for rocky planets in stellar habitable zones is entering an exciting era. With so many…
New constraints on the millimetre emission of six debris disks
Jonathan P. Marshall, S. T. Maddison, E. Thilliez +4
The presence of dusty debris around main sequence stars denotes the existence of planetary systems. Such debris disks are often identified by the presence of excess continuum emiss…
Numerical search for a potential planet sculpting the young disc of HD 115600
E. Thilliez, S. T. Maddison
Radial and azimuthal features (such as disc offsets and eccentric rings) seen in high resolution images of debris discs, provide us with the unique opportunity of finding potential…
Numerical predictions for planets in the debris discs of HD 202628 and HD 207129
E. Thilliez, S. T. Maddison
Resolved debris disc images can exhibit a range of radial and azimuthal structures, including gaps and rings, which can result from planetary companions shaping the disc by their g…
The impact of initial conditions in N-body simulations of debris discs
E. Thilliez, S. T. Maddison
Numerical simulations are a crucial tool to understand the relationship between debris discs and planetary companions. However, simulations throughout the literature have been cond…
MAMBO image of the debris disk around epsilon Eridani : robustness of the azimuthal structure
Jean-Francois Lestrade, Elodie Thilliez
The debris disk closest to Earth is the one around the star epsilon Eridani at a distance of 3.2 pc. It is the prime target for detailed studies of a belt of planetesimals left fro…
A dynamical test for terrestrial planets in the habitable zone of HD 204313
E. Thilliez, L. Jouvin, S. T. Maddison +1
With improvements in exoplanet detection techniques, the number of multiple planet systems discovered is increasing, while the detection of potentially habitable Earth-mass planets…
Tidal stability of giant molecular clouds in the Large Magellanic Cloud
E. Thilliez, S. T. Maddison, A. Hughes +1
Star formation does not occur until the onset of gravitational collapse inside giant molecular clouds. However, the conditions that initiate cloud collapse and regulate the star fo…
A DEBRIS Disk Around The Planet Hosting M-star GJ581 Spatially Resolved with Herschel
J. -F. Lestrade, B. C. Matthews, B. Sibthorpe +17
Debris disks have been found primarily around intermediate and solar mass stars (spectral types A-K) but rarely around low mass M-type stars. We have spatially resolved a debris di…