122 citations · 431 across the 9 of their papers we have counts for
9 papers
The Impact of Phase Equilibrium Cloud Models on GCM Simulations of GJ~1214b
D. A. Christie, N. J. Mayne, R. M. Gillard +4
We investigate the impact of clouds on the atmosphere of GJ~1214b using the radiatively-coupled, phase-equilibrium cloud model {\sc EddySed} coupled to the {\sc Unified Model} gene…
The Impact of Mixing Treatments on Cloud Modelling in 3D Simulations of Hot Jupiters
D. A. Christie, N. J. Mayne, S. Lines +7
We present results of 3D hydrodynamical simulations of HD209458b including a coupled, radiatively-active cloud model ({\sc EddySed}). We investigate the role of the mixing by repla…
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…
Simulating the cloudy atmospheres of HD 209458 b and HD 189733 b with the 3D Met Office Unified Model
S. Lines, N. J. Mayne, Ian A. Boutle +9
To understand and compare the 3D atmospheric structure of HD 209458 b and HD 189733 b, focusing on the formation and distribution of cloud particles, as well as their feedback on t…
Modelling circumbinary protoplanetary disks II. Gas disk feedback on planetesimal dynamical and collisional evolution in the circumbinary systems Kepler-16 and 34
S. Lines, Z. M. Leinhardt, C. Baruteau +2
Aims. We investigate the feasibility of planetesimal growth in circumbinary protoplanetary disks around the observed systems Kepler- 16 and Kepler-34 under the gravitational influe…
Hiding in the Shadows II: Collisional Dust as Exoplanet Markers
Jack Dobinson, Zoe M. Leinhardt, Stefan Lines +3
Observations of the youngest planets (1-10 Myr for a transitional disk) will increase the accuracy of our planet formation models. Unfortunately, observations of such planets…
Modelling circumbinary protoplanetary disks: I. Fluid simulations of the Kepler-16 and 34 systems
S. Lines, Z. M. Leinhardt, C. Baruteau +2
The Kepler mission's discovery of a number of circumbinary planets orbiting close (a_p < 1.1 au) to the stellar binary raises questions as to how these planets could have formed gi…
Numerically Predicted Indirect Signatures of Terrestrial Planet Formation
Zoë M. Leinhardt, Jack Dobinson, Philip J. Carter +1
The intermediate phases of planet formation are not directly observable due to lack of emission from planetesimals. Planet formation is, however, a dynamically active process resul…
Forming Circumbinary Planets: N-body Simulations of Kepler-34
Stefan Lines, Zoe M. Leinhardt, Sijme-Jan Paardekooper +2
Observations of circumbinary planets orbiting very close to the central stars have shown that planet formation may occur in a very hostile environment, where the gravitational pull…