activity
19982026
most citedGeneralised warped disk equations

48 citations · 203 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2026

Negative superhumps in cataclysmic variables driven by retrograde apsidal disk precession

David Vallet, Rebecca G. Martin, Stephen H. Lubow +1

Negative superhumps are photometric modulations in cataclysmic variables with periods slightly shorter than the orbital period. They are usually attributed to retrograde nodal prec…

astro-ph.EP2023★ 8 cited

Coplanar circumbinary planets can be unstable to large tilt oscillations in the presence of an inner polar planet

Anna C. Childs, Rebecca G. Martin, Stephen Lepp +2

Mutually misaligned circumbinary planets may form in a warped or broken gas disc or from later planet-planet interactions. With numerical simulations and analytic estimates we expl…

astro-ph.EP2023★ 15 cited

Polar circumtriple planets and disks can only form close to a triple star

Stephen Lepp, Rebecca G. Martin, Stephen H. Lubow

Observations of protoplanetary disks around binary and triple star systems suggest that misalignments between the orbital plane of the stars and the disks are common. Motivated by…

astro-ph.EP2022★ 2 cited

Formation of super-Earths in icy dead zones around low-mass stars

David Vallet, Anna C. Childs, Rebecca G. Martin +2

While giant planet occurrence rates increase with stellar mass, occurrence rates of close-in super-Earths decrease. This is in contradiction to the expectation that the total mass…

astro-ph.SR2022★ 6 cited

Fast nodal precession of the disc around Pleione requires a broken disc

Rebecca G. Martin, Stephen Lepp

Pleione is a Be star that is in a 218 day orbit with a low-mass binary companion. Recent numerical simulations have shown that a Be star disc can be subject to breaking when materi…

astro-ph.EP2022★ 16 cited

A radial limit on polar circumbinary orbits from general relativity

Stephen Lepp, Rebecca G. Martin, Anna C. Childs

A particle orbiting a misaligned eccentric orbit binary undergoes nodal precession either around the binary angular momentum vector (a circulating orbit) or around a stationary inc…