activity
19962026
most citedA smooth particle hydrodynamics code to model collisions between solid, self-gravitating objects

58 citations · 309 across the 22 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2026

A spectroscopic map of the Galactic centre: Integrated light and dynamical modelling

A. Feldmeier-Krause, T. I. Maindl, G. van de Ven +3

The centre of the Milky Way is occupied by a nuclear star cluster that contains the supermassive black hole Sgr A*. The cluster is embedded in the larger surrounding nuclear stella…

astro-ph.GA2026

Orbital decomposition of the nuclear regions in the early-type galaxy FCC 47: Unveiling the nuclear cluster origin

Julia Lamprecht, Anja Feldmeier-Krause, Mariya Lyubenova +8

Nuclear star clusters (NSCs) are among the densest stellar systems in the Universe and often coexist with supermassive black holes (SMBHs) at galaxy centres. While SMBH formation h…

astro-ph.EP2022★ 8 cited

Residual Neural Networks for the Prediction of Planetary Collision Outcomes

Philip M. Winter, Christoph Burger, Sebastian Lehner +3

Fast and accurate treatment of collisions in the context of modern N-body planet formation simulations remains a challenging task due to inherently complex collision processes. We…

astro-ph.EP2022★ 9 cited

Building Terrestrial Planets: Why results of perfect-merging simulations are not quantitatively reliable approximations to accurate modeling of terrestrial planet formation

Nader Haghighipour, Thomas I. Maindl

Although it is accepted that perfect-merging is not a realistic outcome of collisions, some researchers state that perfect-merging simulations can still be considered as quantitati…

astro-ph.EP2021★ 8 cited

Protoplanet Collisions: Statistical Properties of Ejecta

Samuele Crespi, Ian Dobbs-Dixon, Nikolaos Georgakarakos +4

The last phase of the formation of rocky planets is dominated by collisions among Moon- to Mars-sized planetary embryos. Simulations of this phase need to handle the difficulty of…

astro-ph.EP2020★ 52 cited

Loss and fractionation of noble gas isotopes and moderately volatile elements from planetary embryos and early Venus, Earth and Mars

H. Lammer, M. Scherf, H. Kurokawa +12

Here we discuss the current state of knowledge on how atmospheric escape processes can fractionate noble gas isotopes and moderately volatile rock-forming elements that populate pr…