activity
20032026
most citedThe Formation Mechanism of Gas Giants on Wide Orbits

210 citations · 6.2k across the 148 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.EP2022★ 6 cited

High-resolution resonant portraits of a single-planet white dwarf system

Dimitri Veras, Nikolaos Georgakarakos, Ian Dobbs-Dixon

The dynamical excitation of asteroids due to mean motion resonant interactions with planets is enhanced when their parent star leaves the main sequence. However, numerical investig…

astro-ph.EP2022★ 15 cited

TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved stars

Samuel K. Grunblatt, Nicholas Saunders, Ashley Chontos +27

The fate of planets around rapidly evolving stars is not well understood. Previous studies have suggested that relative to the main sequence population, planets transiting evolved…

astro-ph.EP2022★ 5 cited

Mathematical encoding within multi-resonant planetary systems as SETI beacons

Matthew S. Clement, Sean N. Raymond, Dimitri Veras +1

How might an advanced alien civilization manipulate the orbits within a planetary system to create a durable signpost that communicates its existence? While it is still debated whe…

astro-ph.EP2022

Chaos over Order: Mapping 3D Rotation of Triaxial Asteroids and Minor Planets

Valeri V. Makarov, Alexey Goldin, Alexei V. Tkachenko +2

Celestial bodies approximated with rigid triaxial ellipsoids in a two-body system can rotate chaotically due to the time-varying gravitational torque from the central mass. At smal…

astro-ph.EP2022★ 11 cited

Birth cluster simulations of planetary systems with multiple super-Earths: initial conditions for white dwarf pollution drivers

Katja Stock, Dimitri Veras, Maxwell X. Cai +2

Previous investigations have revealed that eccentric super-Earths represent a class of planets which are particularly effective at transporting minor bodies towards white dwarfs an…

astro-ph.SR2022★ 54 cited

A white dwarf accreting planetary material determined from X-ray observations

Tim Cunningham, Peter J. Wheatley, Pier-Emmanuel Tremblay +4

The atmospheres of a large proportion of white dwarf stars are polluted by heavy elements that are expected to sink out of visible layers on short timescales. This has been interpr…