23 citations · 45 across the 3 of their papers we have counts for
6 papers
The impact of tidal friction evolution on the orbital decay of ultra-short period planets
Jaime A. Alvarado-Montes, Mario Sucerquia, Carolina García-Carmona +3
Unveiling the fate of ultra-short period (USP) planets may help us understand the qualitative agreement between tidal theory and the observed exoplanet distribution. Nevertheless,…
Dust trapping around Lagrangian points in protoplanetary disks
Matias Montesinos, Juan Garrido-Deutelmoser, Johan Olofsson +5
Trojans are defined as objects that share the orbit of a planet at the stable Lagrangian points and . In the Solar System, these bodies show a broad size distribution ra…
Scattered light may reveal the existence of ringed exoplanets
Mario Sucerquia, Jaime A. Alvarado-Montes, Jorge I. Zuluaga +2
Rings around giant exoplanets (hereafter 'exorings') are still a missing planetary phenomenon among the vast number of discovered planets. Despite the fact there exist a large numb…
Can close-in giant exoplanets preserve detectable moons?
Mario Sucerquia, Vanesa Ramírez, Jaime A. Alvarado-Montes +1
Exoplanet discoveries have motivated numerous efforts to find unseen populations of exomoons, yet they have been unsuccessful. A plausible explanation is that most discovered plane…
Ploonets: formation, evolution and detectability of tidally detached exomoons
Mario Sucerquia, Jaime A. Alvarado-Montes, Jorge I. Zuluaga +2
Close-in giant planets represent the most significant evidence of planetary migration. If large exomoons form around migrating giant planets which are more stable (e.g. those in th…
Can we predict the impact conditions of metre-sized meteoroids?
Jorge I. Zuluaga, Pablo A. Cuartas-Restrepo, Jhonatan Ospina +1
Every year, a few metre-sized meteoroids impact the atmosphere of the Earth. Most (if not all) of them are undetectable before the impact. Therefore, predicting where and how they…