7 citations · 7 across the 4 of their papers we have counts for
4 papers
An Inclined, Eccentric Planet and an Inner Debris Disk Could Reproduce AU Mic Structure
Arcelia Hermosillo Ruiz, Ruth Murray-Clay, Meredith A. MacGregor +1
The debris disk orbiting the M star AU Microscopii has a series of large-scale clumps that move away from the star at high velocities above the mid-plane on the southeast side. Two…
Randomness and Retention: Using Weak Mean Motion Resonances to Constrain Neptune's Late-Stage Migration
Arcelia Hermosillo Ruiz, Harriet C. P. Lau, Ruth Murray-Clay
Planet-planetesimal interactions cause a planet to migrate, manifesting as a random walk in semi-major axis. In models for Neptune's migration involving a gravitational upheaval, t…
Can the orbital distribution of Neptune's 3:2 mean motion resonance result from stability sculpting?
Sricharan Balaji, Nihaal Zaveri, Nanae Hayashi +6
We explore a simplified model of the outcome of an early outer Solar System gravitational upheaval during which objects were captured into Neptune's 3:2 mean motion resonance via s…
An Adaptive Optics Census of Companions to Northern Stars Within 25 pc with Robo-AO
Maissa Salama, Carl Ziegler, Christoph Baranec +8
In order to assess the multiplicity statistics of stars across spectral types and populations in a volume-limited sample, we censused nearby stars for companions with Robo-AO. We r…