56 citations · 229 across the 15 of their papers we have counts for
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Binary Planetesimal Formation from Gravitationally Collapsing Pebble Clouds
David Nesvorny, Rixin Li, Jacob B. Simon +4
Planetesimals are compact astrophysical objects roughly 1-1000 km in size, massive enough to be held together by gravity. They can grow by accreting material to become full-size pl…
The dust-to-gas ratio, size distribution, and dust fall-back fraction of comet 67P/Churyumov-Gerasimenko: Inferences from linking the optical and dynamical properties of the inner comae
Raphael Marschall, Johannes Markkanen, Selina-Barbara Gerig +3
In this work, we present results that simultaneously constrain the dust size distribution, dust-to-gas ratio, fraction of dust re-deposition, and total mass production rates for co…
Stability of Jovian Trojans and their collisional families
Timothy R. Holt, David Nesvorny, Jonathan Horner +6
The Jovian Trojans are two swarms of objects located around the L and L Lagrange points. The population is thought to have been captured by Jupiter during the Solar system'…
Limitations in the determination of surface emission distributions on comets through modelling of observational data -- A case study based on Rosetta observations
Raphael Marschall, Ying Liao, Nicolas Thomas +1
The European Space Agency's (ESA) Rosetta mission has returned a vast data set of measurements of the inner gas coma of comet 67P/Churyumov-Gerasimenko. These measurements have bee…
Superparticle Method for Simulating Collisions
David Nesvorny, Andrew N. Youdin, Raphael Marschall +1
For problems in astrophysics, planetary science and beyond, numerical simulations are often limited to simulating fewer particles than in the real system. To model collisions, the…