activity
20062026
most citedA comparative study of disc-planet interaction

446 citations · 4.8k across the 83 of their papers we have counts for

collaborators
Showing 2016 · astro-ph.EPShow all

6 papers · 2 filters

astro-ph.EP2016★ 152 cited

How formation time-scales affect the period dependence of the transition between rocky super-Earths and gaseous sub-Neptunes and implications for

Eric D. Lopez, Ken Rice

One of the most significant advances by NASA's Mission was the discovery of an abundant new population of highly irradiated planets with sizes between the Earth…

astro-ph.EP2016★ 108 cited

Kepler-21b: A rocky planet around a V = 8.25 magnitude star

Mercedes Lopez-Morales, Raphaelle D. Haywood, Jeffrey L. Coughlin +36

HD 179070, aka Kepler-21, is a V = 8.25 F6IV star and the brightest exoplanet host discovered by Kepler. An early detailed analysis by Howell et al. (2012) of the first thirteen mo…

astro-ph.EP2016★ 52 cited

The Orbit and Mass of the Third Planet in the Kepler-56 System

Oderah Justin Otor, Benjamin T. Montet, John Asher Johnson +20

While the vast majority of multiple-planet systems have their orbital angular momentum axes aligned with the spin axis of their host star, Kepler-56 is an exception: its two transi…

astro-ph.EP2016★ 51 cited

Grand challenges in protoplanetary disc modelling

Thomas J. Haworth, John D. Ilee, Duncan H. Forgan +18

The Protoplanetary Discussions conference --- held in Edinburgh, UK, from 7th --11th March 2016 --- included several open sessions led by participants. This paper reports on the di…

astro-ph.EP2016★ 90 cited

A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system

Lars A. Buchhave, Courtney D. Dressing, Xavier Dumusque +35

Kepler-20 is a solar-type star (V = 12.5) hosting a compact system of five transiting planets, all packed within the orbital distance of Mercury in our own Solar System. A transiti…

astro-ph.EP2016★ 39 cited

Directly observing continuum emission from self-gravitating spiral waves

Cassandra Hall, Duncan Forgan, Ken Rice +3

We use a simple, self-consistent, self-gravitating semi-analytic disc model to conduct an examination of the parameter space in which self-gravitating discs may exist. We then use…