Alan P. Boss

TL;DR: In this article, the authors used an N$-body+hydrodynamics simulation of a Milky-Way-like galaxy to identify stars on Sun-like orbits whose environments would produce conditions consistent with those observed.

TL;DR: In this paper, the motions of small solids, ranging from micron-sized dust grains to 100m objects, in the vicinity of a local density enhancement of an isothermal gaseous solar nebula were studied.

TL;DR: In this article, the authors present the first search for these resonant structures in the inner regions of planetary systems by analyzing the light curves of hot Jupiter planetary candidates identified by the Kepler mission and find that at the 90% confidence level, less than 21% of Kepler hot Jupiters create resonant dust clumps that lead and trail the planet by ~90 degrees with optical depths > 5*10^-6.

TL;DR: A transiting Jovian planet orbiting a solar metallicity M4V star was discovered using Transiting Exoplanet Survey Satellite photometry and then confirmed using a combination of precise radial velocities, ground-based photometry, spectra, and speckle imaging as discussed by the authors .

TL;DR: In this article, the authors explored the dynamical phenomenon of mass shedding on the basis of numerical models for a self-gravitating, axisymmetric, polytropic and dissipative protoearth.