activity
20192025
most citedRunaway and walkaway stars from the ONC with Gaia DR2

64 citations · 109 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2025

The impact of internal versus external perturbations on close-in exoplanet architectures

Christina Schoettler, James E Owen

Young planetary systems are subjected to different dynamical effects that can influence their orbital structure over time. In systems with more than one planet, other planets can i…

astro-ph.EP2024

The effect of dynamical interactions in stellar birth environments on the orbits of young close-in planetary systems

Christina Schoettler, James E. Owen

Stars do not form in isolation but together with other stars, and often in a clustered environment. Depending on the initial conditions in these environments, such as initial densi…

astro-ph.EP2023★ 9 cited

Isotopic enrichment of planetary systems from Asymptotic Giant Branch stars

Richard J. Parker, Christina Schoettler

Short-lived radioisotopes, in particular 26-Al and 60-Fe, are thought to contribute to the internal heating of the Earth, but are significantly more abundant in the Solar System co…

astro-ph.SR2020★ 4 cited

Double trouble: Gaia reveals (proto)-planetary systems that may experience more than one dense star-forming environment

Christina Schoettler, Richard J. Parker

Planetary systems appear to form contemporaneously around young stars within young star-forming regions. Within these environments, the chances of survival, as well as the long-ter…

astro-ph.SR2020★ 64 cited

Runaway and walkaway stars from the ONC with Gaia DR2

Christina Schoettler, Jos de Bruijne, Eero Vaher +1

Theory predicts that we should find fast, ejected (runaway) stars of all masses around dense, young star-forming regions. -body simulations show that the number and distribution…

astro-ph.SR2019★ 32 cited

Dynamical evolution of star-forming regions: III. Unbound stars and predictions for Gaia

Christina Schoettler, Richard J. Parker, Becky Arnold +3

We use -body simulations to probe the early phases of the dynamical evolution of star-forming regions and focus on mass and velocity distributions of unbound stars. In this para…