Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR2.7k papers
- Laboratoire d'Astrophysique de BordeauxFR1k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR557 papers
- Institut de Mathématiques de BordeauxFR410 papers
- Laboratoire Bordelais de Recherche en InformatiqueFR390 papers
- Laboratoire Ondes et Matière d'AquitaineFR347 papers
- Institut Polytechnique de BordeauxFR314 papers
- Laboratoire de Physique des deux infinis BordeauxFR314 papers
- Sorbonne UniversitéFR312 papers
- CEA Paris-SaclayFR309 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR299 papers
- Astrophysique, Instrumentation et ModélisationFR278 papers
22 papers · 2 filters
Excitation and depletion of the asteroid belt in the early instability scenario
Matthew S. Clement, Sean N. Raymond, Nathan A. Kaib
Containing only a few percent the mass of the moon, the current asteroid belt is around three to four orders of magnitude smaller that its primordial mass inferred from disk models…
An optical transmission spectrum of the ultra-hot Jupiter WASP-33b. First indication of AlO in an exoplanet
C. von Essen, M. Mallonn, L. Welbanks +4
There has been increasing progress toward detailed characterization of exoplanetary atmospheres, in both observations and theoretical methods. Improvements in observational facilit…
Global climate modeling of Saturn's atmosphere. Part II: multi-annual high-resolution dynamical simulations
Aymeric Spiga, Sandrine Guerlet, Ehouarn Millour +9
The Cassini mission unveiled the intense and diverse activity in Saturn's atmosphere: banded jets, waves, vortices, equatorial oscillations. To set the path towards a better unders…
Can Moons Have Moons?
Juna A. Kollmeier, Sean N. Raymond
Each of the giant planets within the Solar System has large moons but none of these moons have their own moons (which we call ). By analogy with studies of moons ar…
Modeling the albedo of Earth-like magma ocean planets with H2O-CO2 atmospheres
William Pluriel, Emmanuel Marcq, Martin Turbet
During accretion, the young rocky planets are so hot that they become endowed with a magma ocean. From that moment, the mantle convective thermal flux control the cooling of the pl…
Continuous reorientation of synchronous terrestrial planets controlled by mantle convection
Jérémy Leconte
A large fraction of known rocky exoplanets are expected to have been spun-down to a state of synchronous rotation, including temperate ones. Studies about the atmospheric and surfa…
Temperature, Mass and Turbulence: A Spatially Resolved Multi-Band Non-LTE Analysis of CS in TW~Hya
Richard Teague, Thomas Henning, Stephane Guilloteau +6
Observations of multiple rotational transitions from a single molecule allow for unparalleled constraints on the physical conditions of the emitting region. We present an analysis…
Evolution of Earth-like extrasolar planetary atmospheres: Assessing the atmospheres and biospheres of early Earth analog planets with a coupled atmosphere biogeochemical model
S. Gebauer, J. L. Grenfell, J. W. Stock +4
Understanding the evolution of Earth and potentially habitable Earth-like worlds is essential to fathom our origin in the Universe. The search for Earth-like planets in the habitab…
The 0.8-4.5m broadband transmission spectra of TRAPPIST-1 planets
E. Ducrot, M. Sestovic, B. M. Morris +18
The TRAPPIST-1 planetary system represents an exceptional opportunity for the atmospheric characterization of temperate terrestrial exoplanets with the upcoming James Webb Space Te…
Vortex survival in 3D self-gravitating accretion discs
Min-Kai Lin, Arnaud Pierens
Large-scale, dust-trapping vortices may account for observations of asymmetric protoplanetary discs. Disc vortices are also potential sites for accelerated planetesimal formation b…
On the evolution of vortices in massive protoplanetary discs
Arnaud Pierens, Min-Kai Lin
It is expected that a pressure bump can be formed at the inner edge of a dead-zone, and where vortices can develop through the Rossby Wave Instability (RWI). It has been suggested…
Migration-driven diversity of super-Earth compositions
Sean N. Raymond, Thibault Boulet, Andre Izidoro +2
A leading model for the origin of super-Earths proposes that planetary embryos migrate inward and pile up on close-in orbits. As large embryos are thought to preferentially form be…
Mars' Growth Stunted by an Early Giant Planet Instability
Matthew S. Clement, Nathan A. Kaib, Sean N. Raymond +1
Many dynamical aspects of the solar system can be explained by the outer planets experiencing a period of orbital instability sometimes called the Nice Model. Though often correlat…
Identifying inflated super-Earths and photo-evaporated cores
Daniel Carrera, Eric B. Ford, Andre Izidoro +3
We present empirical evidence, supported by a planet formation model, to show that the curve approximates the location of the so-called pho…
Orbital alignment of circumbinary planets that form in misaligned circumbinary discs: the case of Kepler-413b
Arnaud Pierens, Richard P. Nelson
Although most of the circumbinary planets detected by the Kepler spacecraft are on orbits that are closely aligned with the binary orbital plane, the systems Kepler-413 and Kepler-…
Formation of Terrestrial Planets
Andre Izidoro, Sean N. Raymond
The past decade has seen major progress in our understanding of terrestrial planet formation. Yet key questions remain. In this review we first address the growth of 100 km-scale p…
Interstellar object 'Oumuamua as an extinct fragment of an ejected cometary planetesimal
Sean N. Raymond, Philip J. Armitage, Dimitri Veras
'Oumuamua was discovered passing through our Solar System on a hyperbolic orbit. It presents an apparent contradiction, with colors similar to those of volatile-rich Solar System b…
The Transiting Exoplanet Community Early Release Science Program for JWST
Jacob L. Bean, Kevin B. Stevenson, Natalie M. Batalha +99
The James Webb Space Telescope (JWST) presents the opportunity to transform our understanding of planets and the origins of life by revealing the atmospheric compositions, structur…
Photochemistry, mixing and transport in Jupiter's stratosphere constrained by Cassini
Vincent Hue, Franck Hersant, Thibault Cavalié +2
We aim at constraining the diffusive and advective transport processes in Jupiter's stratosphere. The IR spectrum recorded by Cassini/CIRS during the Jupiter flyby contains the fin…
The Delivery of Water During Terrestrial Planet Formation
David P. O'Brien, Andre Izidoro, Seth A. Jacobson +2
The planetary building blocks that formed in the terrestrial planet region were likely very dry, yet water is comparatively abundant on Earth. We review the various mechanisms prop…
Formation of terrestrial planets in eccentric and inclined giant planet systems
Sotiris Sotiriadis, Anne-Sophie Libert, Sean N. Raymond
Evidence of mutually inclined planetary orbits has been reported for giant planets these last years. Here we aim to study the impact of eccentric and inclined massive giant planets…
Early 2017 observations of TRAPPIST-1 with
Laetitia Delrez, Michael Gillon, Amaury H. M. J. Triaud +14
The recently detected TRAPPIST-1 planetary system, with its seven planets transiting a nearby ultracool dwarf star, offers the first opportunity to perform comparative exoplanetolo…