output
20022026
most citedThe LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release

654 citations

Showing astro-ph.EPShow all

16 papers · 1 filter

astro-ph.EP20261 cited

Evolution and Observable Properties of Rocky Planet Atmospheres

Marie-Luise Steinmeyer, Lena Noack, Philipp Baumeister +9

The atmospheric composition of rocky exoplanets offers an important tool for constraining the properties of the interior of this type of planet, beyond what is possible from measur…

astro-ph.EP2026

High-Latitude Zonal Jets in the Martian Upper Atmosphere Driven by Non-Orographic Gravity Waves

Jiandong Liu, François Forget, Ehouarn Millour +2

We investigate thermosphere responses to non-orographic gravity waves (GWs) using wind measurements from the Neutral Gas and Ion Mass Spectrometer onboard the Mars Atmosphere and V…

astro-ph.EP20253 cited

A Stochastic Parameterization of Non-Orographic Gravity Waves Induced Mixing for Mars Planetary Climate Model

Jiandong Liu, Ehouarn Millour, François Forget +2

This paper presents a formalism of mixing induced by non-orographic gravity waves (GWs) to integrate with the stochastic GWs scheme in the Mars Planetary Climate Model. We derive t…

astro-ph.EP2024

Planetesimal gravitational collapse in a gaseous environment: Thermal and dynamic evolution

P. Segretain, H. Méheut, M. Moreira +3

Planetesimal formation models often invoke the gravitational collapse of pebble clouds to overcome various barriers to grain growth and propose processes to concentrate particles s…

astro-ph.EP202413 cited

Star-Planet Interactions in the Radio Domain: Prospect for Their Detection

Philippe Zarka

All types of interaction of a magnetized plasma flow with an obstacle (magnetized or not) are considered, and those susceptible to produce a radio signature are identified. The rol…

astro-ph.EP202313 cited

Narrow loophole for H2-dominated atmospheres on habitable rocky planets around M dwarfs

Renyu Hu, Fabrice Gaillard, Edwin Kite

Habitable rocky planets around M dwarfs that have H2-dominated atmospheres, if they exist, would permit characterizing habitable exoplanets with detailed spectroscopy using JWST, o…