activity
20152023
most citedThe chemical evolution of the solar neighbourhood for planet-hosting stars

15 citations · 18 across the 2 of their papers we have counts for

collaborators

7 papers

cs.CV2023★ 3 cited

DECO: Dense Estimation of 3D Human-Scene Contact In The Wild

Shashank Tripathi, Agniv Chatterjee, Jean-Claude Passy +3

Understanding how humans use physical contact to interact with the world is key to enabling human-centric artificial intelligence. While inferring 3D contact is crucial for modelin…

astro-ph.GA2023★ 15 cited

The chemical evolution of the solar neighbourhood for planet-hosting stars

Marco Pignatari, Thomas C. L. Trueman, Kate A. Womack +13

Theoretical physical-chemical models for the formation of planetary systems depend on data quality for the Sun's composition, that of stars in the solar neighbourhood, and of the e…

astro-ph.SR2017

The effect of binding energy and resolution in simulations of the common envelope binary interaction

Roberto Iaconi, Orsola De Marco, Jean-Claude Passy +1

The common envelope binary interaction remains one of the least understood phases in the evolution of compact binaries, including those that result in Type Ia supernovae and in mer…

astro-ph.SR2017

Common envelope light-curves - I. grid-code module calibration

Pablo Galaviz, Orsola De Marco, Jean-Claude Passy +2

The common envelope binary interaction occurs when a star transfers mass onto a companion that cannot fully accrete it. The interaction can lead to a merger of the two objects or t…

astro-ph.SR2016

The effect of a wider initial separation on common envelope binary interaction simulations

Roberto Iaconi, Thomas Reichardt, Jan Staff +5

We present hydrodynamic simulations of the common envelope binary interaction between a giant star and a compact companion carried out with the adaptive mesh refinement code ENZO a…

astro-ph.SR2016

Hydrodynamic Simulations of the Interaction between Giant Stars and Planets

Jan E. Staff, Orsola De Marco, Peter Wood +2

We present the results of hydrodynamic simulations of the interaction between a 10 Jupiter mass planet and a red or asymptotic giant branch stars, both with a zero-age main sequenc…