activity
19972026
most citedMigration and the formation of systems of hot super-Earths and Neptunes

372 citations · 2.4k across the 42 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

12 papers · 1 filter

astro-ph.EP2020★ 5 cited

Tidally induced stellar oscillations: converting modelled oscillations excited by hot Jupiters into observables

Andrew Bunting, Caroline Terquem

We calculate the conversion from non-adiabatic, non-radial oscillations tidally induced by a hot Jupiter on a star to observable spectroscopic and photometric signals. Models with…

astro-ph.EP2019★ 11 cited

Non-adiabatic tidal oscillations induced by a planetary companion

Andrew Bunting, John C. B. Papaloizou, Caroline Terquem

We calculate the dynamical tides raised by a close planetary companion on non-rotating stars of and . Using the Henyey method, we sol…

astro-ph.EP2018★ 30 cited

First-order mean motion resonances in two-planet systems: general analysis and observed systems

Caroline Terquem, John Papaloizou

This paper focuses on two-planet systems in a first-order mean motion resonance and undergoing type-I migration in a disc. We present a detailed analysis of the resonance…

astro-ph.EP2017★ 74 cited

The TRAPPIST-1 system: Orbital evolution, tidal dissipation, formation and habitability

John C. B. Papaloizou, Ewa Szuszkiewicz, Caroline Terquem

We study the dynamical evolution of the TRAPPIST-1 system under the influence of orbital circularization through tidal interaction with the central star. We find that systems with…

astro-ph.EP2016★ 4 cited

On the formation of planetary systems in photoevaporating transition discs

Caroline Terquem

In protoplanetary discs, planetary cores must be at least 0.1 earth mass at 1 au for migration to be significant; this mass rises to 1 earth mass at 5 au. Planet formation models i…

astro-ph.EP2014★ 28 cited

On the formation of the Kepler-10 planetary system

Caroline Terquem

In this paper, we investigate the conditions required for the 3 and 17 Earth mass solid planets in the Kepler-10 system to have formed through collisions and mergers within an init…