244 citations · 4k across the 91 of their papers we have counts for
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Long-term evolution of three-planet systems to the post-Main Sequence and beyond
Alexander Mustill, Dimitri Veras, Eva Villaver
We study the stability of systems of three giant planets orbiting 3 - 8 M_Sol stars at orbital distances of >10 au as the host star ages through the Main Sequence (MS) and well int…
Main-sequence progenitor configurations of the NN Ser candidate circumbinary planetary system are dynamically unstable
Alexander J Mustill, Jonathan P Marshall, Eva Villaver +4
Recent observations of the NN Serpentis post-common envelope binary system have revealed eclipse timing variations that have been attributed to the presence of two Jovian-mass exop…
A Detailed Dynamical Investigation of the Proposed QS Virginis Planetary System
Jonathan Horner, Robert A Wittenmyer, Tobias C Hinse +3
In recent years, a number of planetary systems have been proposed to orbit evolved binary star systems. The presence of planets is invoked to explain observed variations in the tim…
Herschel's "Cold Debris Disks": Background Galaxies or Quiescent Rims of Planetary Systems?
A. V. Krivov, C. Eiroa, T. Löhne +24
(abridged) Infrared excesses associated with debris disk host stars detected so far peak at wavelengths around ~100μm or shorter. However, six out of 31 excess sources in the Hersc…
A simple scaling for the minimum instability time-scale of two widely spaced planets
Dimitri Veras, Alexander J. Mustill
Long-term instability in multi-planet exosystems is a crucial consideration when confirming putative candidates, analyzing exoplanet populations, constraining the age of exosystems…
Simulations of two-planet systems through all phases of stellar evolution: implications for the instability boundary and white dwarf pollution
Dimitri Veras, Alexander J. Mustill, Amy Bonsor +1
Exoplanets have been observed at many stages of their host star's life, including the main sequence (MS), subgiant and red giant branch stages. Also, polluted white dwarfs (WDs) li…