64 citations · 140 across the 8 of their papers we have counts for
8 papers
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…
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…
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…
Using deep generative neural networks to account for model errors in Markov chain Monte Carlo inversion
Shiran Levy, Jürg Hunziker, Eric Laloy +2
Most geophysical inverse problems are nonlinear and rely upon numerical forward solvers involving discretization and simplified representations of the underlying physics. As a resu…
Constraining the initial conditions of NGC 2264 using ejected stars found in Gaia DR2
Christina Schoettler, Richard J. Parker, Jos de Bruijne
Fast, ejected stars have been found around several young star-forming regions, such as the Orion Nebula Cluster (ONC). These ejected stars can be used to constrain the initial dens…
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…
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…
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…