activity
20062026
most citedAn extrasolar planetary system with three Neptune-mass planets

387 citations · 3.3k across the 89 of their papers we have counts for

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Showing 2017Show all

7 papers · 1 filter

astro-ph.EP2017★ 20 cited

On the coplanar eccentric non restricted co-orbital dynamics

A. Leleu, P. Robutel, A. C. M. Correia

We study the phase space of eccentric coplanar co-orbitals in the non-restricted case. Departing from the quasi-circular case, we describe the evolution of the phase space as the e…

astro-ph.EP2017★ 36 cited

The TROY project: Searching for co-orbital bodies to known planets. I. Project goals and first results from archival radial velocity

J. Lillo-Box, D. Barrado, P. Figueira +5

The detection of Earth-like planets, exocomets or Kuiper belts show that the different components found in the solar system should also be present in other planetary systems. Troja…

astro-ph.EP2017★ 18 cited

Chaotic dynamics in the (47171) Lempo triple system

Alexandre C. M. Correia

We investigate the dynamics of the (47171) Lempo triple system, also known by 1999TC. We derive a full 3D -body model that takes into account the orbital and spin evoluti…

astro-ph.EP2017★ 12 cited

Lidov-Kozai stability regions in the alpha Centauri system

C. A. Giuppone, A. C. M. Correia

The stability of planets in the alpha-Centauri AB stellar system has been studied extensively. However, most studies either focus on the orbital plane of the binary or consider inc…

astro-ph.IM2017★ 52 cited

Theia: Faint objects in motion or the new astrometry frontier

The Theia Collaboration, Celine Boehm, Alberto Krone-Martins +96

In the context of the ESA M5 (medium mission) call we proposed a new satellite mission, Theia, based on relative astrometry and extreme precision to study the motion of very faint…

astro-ph.EP2017★ 30 cited

Detection of co-orbital planets by combining transit and radial-velocity measurements

Adrien Leleu, Philippe Robutel, Alexandre C M Correia +1

Co-orbital planets have not yet been discovered, although they constitute a frequent by-product of planetary formation and evolution models. This lack may be due to observational b…