activity
20182020
collaborators

11 papers

astro-ph.GA2020

Time evolution of gaps in stellar streams in axisymmetric Stäckel potentials

Helmer H. Koppelman, Amina Helmi

When a subhalo interacts with a cold stellar stream it perturbs its otherwise nearly smooth distribution of stars, and this leads to the creation of a gap. The properties of such g…

astro-ph.GA2020

Frequencies, chaos and resonances: a study of orbital parameters of nearby thick disc and halo stars

Helmer H. Koppelman, Jorrit H. J. Hagen, Amina Helmi

We study the distribution of nearby thick disc and halo stars in subspaces defined by their characteristic orbital parameters. Our aim is to establish the origin of the structure r…

astro-ph.GA2020

Galactic potential constraints from clustering in action space of combined stellar stream data

Stella Reino, Elena M. Rossi, Robyn E. Sanderson +4

Stream stars removed by tides from their progenitor satellite galaxy or globular cluster act as a group of test particles on neighboring orbits, probing the gravitational field of…

astro-ph.GA2020

A massive mess: When a large dwarf and a Milky Way-like galaxy merge

Helmer H. Koppelman, Roy O. Y. Bos, Amina Helmi

Circa 10 billion years ago the Milky Way merged with a massive satellite, Gaia-Enceladus. To gain insight into the properties of its debris we analyse in detail the suite of simula…

astro-ph.GA2019

Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history

Helmer H. Koppelman, Amina Helmi, Davide Massari +2

Aims. Several kinematic and chemical substructures have been recently found amongst Milky Way halo stars with retrograde motions. It is currently unclear how these various structur…

astro-ph.GA2019

Origin of the system of globular clusters in the Milky Way

Davide Massari, Helmer H. Koppelman, Amina Helmi

. The assembly history experienced by the Milky Way is currently being unveiled thanks to the data provided by the mission. It is likely that the globular cluster s…