activity
20102024
most citedEarly UV Ingress in WASP-12b: Measuring Planetary Magnetic Fields

187 citations · 662 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2024

Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815

Angelica Psaridi, Hugh Osborn, François Bouchy +130

We present the discovery and characterization of two warm mini-Neptunes transiting the K3V star TOI-815 in a K-M binary system. Analysis of the spectra and rotation period reveal i…

astro-ph.SR2022★ 23 cited

MOVES V. Modelling star-planet magnetic interactions of HD 189733

A. Strugarek, R. Fares, V. Bourrier +10

Magnetic interactions between stars and close-in planets may lead to a detectable signal on the stellar disk. HD 189733 is one of the key exosystems thought to harbor magnetic inte…

astro-ph.EP2020★ 39 cited

MOVES III. Simultaneous X-ray and ultraviolet observations unveiling the variable environment of the hot Jupiter HD 189733b

V. Bourrier, P. J. Wheatley, A. Lecavelier des Etangs +8

In this third paper of the MOVES (Multiwavelength Observations of an eVaporating Exoplanet and its Star) programme, we combine Hubble Space Telescope far-ultraviolet observations w…

astro-ph.SR2019★ 38 cited

MOVES II. Tuning in to the radio environment of HD189733b

R. D. Kavanagh, A. A. Vidotto, D. Ó Fionnagáin +7

We present stellar wind modelling of the hot Jupiter host HD189733, and predict radio emission from the stellar wind and the planet, the latter arising from the interaction of the…

astro-ph.SR2017★ 44 cited

MOVES I. The evolving magnetic field of the planet-hosting star HD189733

R. Fares, V. Bourrier, A. A. Vidotto +9

HD189733 is an active K dwarf that is, with its transiting hot Jupiter, among the most studied exoplanetary systems. In this first paper of the Multiwavelength Observations of an e…

astro-ph.SR2011★ 40 cited

Shock formation around planets orbiting M-dwarf stars

A. A. Vidotto, J. Llama, M. Jardine +2

Bow shocks can be formed around planets due to their interaction with the coronal medium of the host stars. The net velocity of the particles impacting on the planet determines the…