activity
20132017
most citedHeartbeat Stars, Tidally Excited Oscillations, and Resonance Locking

140 citations · 389 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.EP201712 cited

How Cassini Can Constrain Tidal Dissipation in Saturn

Jing Luan, Jim Fuller, Eliot Quataert

Tidal dissipation inside giant planets is important for the orbital evolution of their natural satellites. It is conventionally treated by parameterized equilibrium tidal theory, i…

astro-ph.SR201725 cited

The Pseudosynchronization of Binary Stars Undergoing Strong Tidal Interactions

Mara Zimmerman, Susan Thompson, Fergal Mullally +3

Eccentric binaries known as heartbeat stars experience strong dynamical tides as the stars pass through periastron, providing a laboratory to study tidal interactions. We measure t…

astro-ph.SR2017140 cited

Heartbeat Stars, Tidally Excited Oscillations, and Resonance Locking

Jim Fuller

Heartbeat stars are eccentric binary stars in short period orbits whose light curves are shaped by tidal distortion, reflection, and Doppler beaming. Some heartbeat stars exhibit t…

astro-ph.SR201735 cited

Accelerated Tidal Circularization Via Resonance Locking in KIC 8164262

Jim Fuller, Kelly Hambleton, Avi Shporer +2

Tidal dissipation in binary star and planetary systems is poorly understood. Fortunately, eccentric binaries known as heartbeat stars often exhibit tidally excited oscillations, pr…

astro-ph.SR201751 cited

KIC 8164262: a Heartbeat Star Showing Tidally Induced Pulsations with Resonant Locking

K. Hambleton, J. Fuller, S. Thompson +8

We present the analysis of KIC 8164262, a heartbeat star with a high-amplitude (~1 mmag), tidally resonant pulsation (a mode in resonance with the orbit) at 229 times the orbital f…

astro-ph.SR201754 cited

The Most Massive Heartbeat: An In-depth Analysis of ι Orionis

Herbert Pablo, N. D. Richardson, J. Fuller +17

ι Ori is a well studied massive binary consisting of an O9 III + B1 III/IV star. Due to its high eccentricity (e = 0.764) and short orbital period (P orb = 29.13376 d), it has been…