output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2013 · astro-ph.EPShow all

23 papers · 2 filters

astro-ph.EP2013★ 72 cited

The atmospheric chemistry of the warm Neptune GJ 3470b: influence of metallicity and temperature on the CH4/CO ratio

Olivia Venot, Marcelino Agundez, Franck Selsis +2

Current observation techniques are able to probe the atmosphere of some giant exoplanets and get some clues about their atmospheric composition. However, the chemical compositions…

astro-ph.EP2013★ 70 cited

The puzzling chemical composition of GJ 436b's atmosphere: influence of tidal heating on the chemistry

M. Agundez, O. Venot, F. Selsis +1

The dissipation of the tidal energy deposited on eccentric planets may induce a heating of the planet that affects its atmospheric thermal structure. Here we study the influence of…

astro-ph.EP2013★ 99 cited

Terrestrial Planet Formation at Home and Abroad

Sean N. Raymond, Eiichiro Kokubo, Alessandro Morbidelli +2

We review the state of the field of terrestrial planet formation with the goal of understanding the formation of the inner Solar System and low-mass exoplanets. We review the dynam…

astro-ph.EP2013★ 72 cited

First submillimeter observation of CO in the stratosphere of Uranus

T. Cavalié, R. Moreno, E. Lellouch +8

Context. Carbon monoxide (CO) has been detected in all Giant Planets and its origin is both internal and external in Jupiter and Neptune. Despite its first detection in Uranus a de…

astro-ph.EP2013★ 18 cited

Solar System Moons as Analogs for Compact Exoplanetary Systems

Stephen R. Kane, Natalie R. Hinkel, Sean N. Raymond

The field of exoplanetary science has experienced a recent surge of new systems that is largely due to the precision photometry provided by the Kepler mission. The latest discoveri…

astro-ph.EP2013★ 25 cited

Making giant planet cores: convergent migration and growth of planetary embryos in non-isothermal discs

Arnaud Pierens, Christophe Cossou, Sean Raymond

Earth-mass bodies are expected to undergo Type I migration directed either inward or outward depending on the thermodynamical state of the protoplanetary disc. Zones of convergent…