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- Publications
- Influence
MAMBO image of the debris disk around epsilon Eridani : robustness of the azimuthal structure
- J. Lestrade, E. Thilliez
- Physics
- 10 March 2015
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 from the early phase… Expand
A DEBRIS disk around the planet hosting M-star GJ 581 spatially resolved with Herschel
- J. Lestrade, B. Matthews, +17 authors D. Wilner
- Physics
- 20 November 2012
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 disk around the… Expand
New constraints on the millimetre emission of six debris discs
- J. Marshall, S. Maddison, +4 authors W. Holland
- Physics, Geology
- 17 March 2017
The presence of dusty debris around main-sequence stars denotes the existence of planetary systems. Such debris discs are often identified by the presence of excess continuum emission at infrared and… Expand
Numerical search for a potential planet sculpting the young disc of HD 115600
- E. Thilliez, S. Maddison
- Physics
- 22 September 2016
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 planetary… Expand
Numerical predictions for planets in the debris discs of HD 202628 and HD 207129
- E. Thilliez, S. Maddison
- Physics
- 10 January 2016
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 gravitational… Expand
Measuring traffic congestion: An approach based on learning weighted inequality, spread and aggregation indices from comparison data
- G. Beliakov, M. Gagolewski, +4 authors Rajesh Vasa
- Mathematics, Computer Science
- Appl. Soft Comput.
- 13 July 2017
TLDR
Stable habitable zones of single Jovian planet systems
- M. Agnew, S. Maddison, E. Thilliez, J. Horner
- Physics
- 19 June 2017
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 exoplanetary… Expand
A dynamical test for terrestrial planets in the habitable zone of HD 204313
- E. Thilliez, L. Jouvin, S. Maddison, J. Horner,
- Geology, Physics
- 1 February 2014
With improvements in exoplanet detection techniques, the number of multiple planet systems discovered is increasing, while the detection of potentially habitable Earth-mass planets remains… Expand
Tidal Stability of Giant Molecular Clouds in the Large Magellanic Cloud
- E. Thilliez, S. Maddison, A. Hughes, T. Wong
- Physics
- 24 October 2013
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 formation process… Expand