27 citations · 46 across the 5 of their papers we have counts for
7 papers
Production of hot Jupiter candidates from high-eccentricity mechanisms for different initial planetary mass configurations
H. Garzón, Adrián Rodríguez, G. C. de Elía
Hot Jupiters (HJs) are giant planets with orbital periods of the order of a few days with semimajor axis within 0.1 au. Several theories have been invoked in order to explain…
Water worlds in N-body simulations with fragmentation in systems without gaseous giants
Agustín Dugaro, Gonzalo C. de Elía, Luciano A. Darriba
We analyze the formation and evolution of terrestrial-like planets around solar-type stars in the absence of gaseous giants. In particular, we focus on the physical and dynamical p…
The inverse Lidov-Kozai resonance for an outer test particle due to an eccentric perturber
Gonzalo Carlos de Elía, Macarena Zanardi, Agustín Dugaro +1
We analyze the behavior of the argument of pericenter of an outer particle in the elliptical restricted three-body problem, focusing on the inverse Lidov-Kozai resonance. Fir…
Role of gaseous giants in the dynamical evolution of terrestrial planets and water delivery in the habitable zone
Mariana B. Sánchez, Gonzalo C. de Elía, Luciano A. Darriba
In the present research, we study the effects of a single giant planet in the dynamical evolution of water-rich embryos and planetesimals, located beyond the snow line of systems a…
The role of the general relativity on icy body reservoirs under the effects of an inner eccentric Jupiter
Macarena Zanardi, Gonzalo Carlos de Elía, Romina P. Di Sisto +1
Recent studies have analyzed the dynamical evolution of outer small body populations under the effects of an eccentric inner massive perturber. Such outer reservoirs are composed o…
Migrating Jupiter up to the habitable zone: Earth-like planet formation and water delivery
L. A. Darriba, G. C. de Elía, O. M. Guilera +1
Several observational works have shown the existence of Jupiter-mass planets covering a wide range of semi-major axes around Sun-like stars. We aim to analyse the planetary formati…