210 citations · 6.2k across the 148 of their papers we have counts for
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Secular Evolution of HD 12661: A System Caught at an Unlikely Time
Dimitri Veras, Eric B. Ford
The eccentricity evolution of multiple planet systems can provide valuable constraints on planet formation models. Unfortunately, the inevitable uncertainties in the current orbita…
Characterizing the Orbital Eccentricities of Transiting Extrasolar Planets with Photometric Observations
Eric B. Ford, Samuel N. Quinn, Dimitri Veras
The discovery of over 200 extrasolar planets with the radial velocity (RV) technique has revealed that many giant planets have large eccentricities, in striking contrast with most…
A resonant-term-based model including a nascent disk, precession, and oblateness: application to GJ 876
Dimitri Veras
Investigations of two resonant planets orbiting a star or two resonant satellites orbiting a planet often rely on a few resonant and secular terms in order to obtain a representati…
Influence of massive planet scattering on nascent terrestrial planets
Dimitri Veras, Philip J. Armitage
In most extrasolar planetary systems, the present orbits of known giant planets admit the existence of stable terrestrial planets. Those same giant planets, however, have typically…
The Dynamics of Two Massive Planets on Inclined Orbits
Dimitri Veras, Philip J. Armitage
The significant orbital eccentricities of most giant extrasolar planets may have their origin in the gravitational dynamics of initially unstable multiple planet systems. In this w…
Stability of Terrestrial Planets in the Habitable Zone of Gl 777 A, HD 72659, Gl 614, 47 Uma and HD 4208
N. Asghari, C. Broeg, L. Carone +37
We have undertaken a thorough dynamical investigation of five extrasolar planetary systems using extensive numerical experiments. The systems Gl 777 A, HD 72659, Gl 614, 47 Uma and…
Migration of extrasolar planets to large orbital radii
Dimitri Veras, Philip J. Armitage
Observations of structure in circumstellar debris discs provide circumstantial evidence for the presence of massive planets at large (several tens of au) orbital radii, where the t…