activity
20042020
most citedCapture and migration of Jupiter and Saturn in mean motion resonance in a gaseous protoplanetary disc

16 citations · 22 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.EP202016 cited

Capture and migration of Jupiter and Saturn in mean motion resonance in a gaseous protoplanetary disc

Raul O. Chametla, Gennaro D'Angelo, Mauricio Reyes-Ruiz +1

We study the dynamical evolution of Jupiter and Saturn embedded in a gaseous, solar-nebula-type disc by means of hydrodynamics simulations with the FARGO2D1D code. We study the evo…

astro-ph.EP2020

Size and Shape Constraints of (486958) Arrokoth from Stellar Occultations

Marc W. Buie, Simon B. Porter, Peter Tamblyn +130

We present the results from four stellar occultations by (486958) Arrokoth, the flyby target of the New Horizons extended mission. Three of the four efforts led to positive detecti…

astro-ph.EP20195 cited

First Results from the rapid-response spectrophotometric characterization of Near-Earth Objects

Samuel Navarro-Meza, Michael Mommert, David Trilling +6

As part of our multi-observatory, multi-filter campaign, we present \rmi color observations of 82 Near-Earth Objects (NEOs) obtained with the RATIR instrument on the 1.5m robotic t…

astro-ph.EP2016

First Results from the Rapid-Response Spectrophotometric Characterization of Near-Earth Objects using UKIRT

M. Mommert, D. E. Trilling, D. Borth +7

Using the Wide Field Camera for the United Kingdom Infrared Telescope, we measure the near-infrared colors of near-Earth objects (NEOs) in order to put constraints on their taxonom…

astro-ph20081 cited

Numerical Simulation of the Viscous-like Flow in and Around the Plasma Tail of a Comet

M. Reyes-Ruiz, H. Perez-de-Tejada, H. Aceves +1

We model the interaction of the solar wind with the plasma tail of a comet by means of numerical simulations, taking into account the effects of viscous-like forces.A 2D hydrodynam…

astro-ph2004

Constraining the Magnetic Effects on HI Rotation Curves and the Need for Dark Halos

F. J. Sanchez-Salcedo, M. Reyes-Ruiz

The density profiles of dark halos are usually inferred from the rotation curves of disk galaxies based on the assumption that the gas is a good tracer of the gravitational potenti…