activity
19982023
most citedHow Observations of Circumstellar Disk Asymmetries Can Reveal Hidden Planets: Pericenter Glow and its Application to the HR 4796 Disk

409 citations · 746 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.EP2023

Deconvolving the complex structure of the asteroid belt

Stanley F. Dermott, Dan Li, Apostolos A. Christou

The asteroid belt is a unique source of information on some of the most important questions facing solar system science. These questions include the sizes, numbers, types and orbit…

astro-ph.EP2022★ 4 cited

Chaotic diffusion of asteroids in the exterior 1:2 mean motion resonance with Mars

Apostolos A. Christou, Stanley F. Dermott, Dan Li

The inner asteroid belt between 2.1 and 2.5 au is of particular dynamical significance because it is the dominant source of both chondritic meteorites and near-Earth asteroids. Thi…

astro-ph.EP2020★ 47 cited

The common origin of family and non-family asteroids

Stanley F. Dermott, Apostolos A. Christou, Dan Li +2

All asteroids are currently classified as either family, originating from the disruption of known bodies, or non-family. An outstanding question is the origin of these non-family a…

astro-ph.EP2020★ 20 cited

Dynamical evolution of the inner asteroid belt

Stanley F. Dermott, Dan Li, Apostolos A. Christou +3

A determination of the dynamical evolution of the asteroid belt is difficult because the asteroid belt has evolved since the time of asteroid formation through mechanisms that incl…

astro-ph.EP2009★ 39 cited

Three years of Ulysses dust data: 2005 to 2007

Harald Krüger, V. Dikarev, B. Anweiler +16

The Ulysses spacecraft has been orbiting the Sun on a highly inclined ellipse since it encountered Jupiter in February 1992. Since then it made almost three revolutions about the S…

astro-ph.EP2009★ 14 cited

Galileo dust data from the jovian system: 2000 to 2003

Harald Krüger, D. Bindschadler, S. F. Dermott +17

The Galileo spacecraft was orbiting Jupiter between Dec 1995 and Sep 2003. The Galileo dust detector monitored the jovian dust environment between about 2 and 370 R_J (jovian radiu…