activity
20142018
most citedSizes of protoplanetary discs after star-disc encounters

82 citations · 220 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2018★ 15 cited

Creating retrogradely orbiting planets by prograde stellar fly-bys

Andreas Breslau, Susanne Pfalzner

Several planets have been found that orbit their host star on retrograde orbits (spin-orbit angle ϕ > 90°). Currently, the largest measured projected angle between the orbital angu…

astro-ph.EP2017★ 18 cited

From star-disc encounters to numerical solutions for a subset of the restricted three-body problem

Andreas Breslau, Kirsten Vincke, Susanne Pfalzner

Various astrophysical processes are known, where the fly-by of a massive object affects matter initially supported against gravity by rotation. Examples are perturbations of galaxi…

astro-ph.EP2016★ 29 cited

Effects of inclined star-disk encounter on protoplanetary disk size

Asmita Bhandare, Andreas Breslau, Susanne Pfalzner

Most, if not all, young stars are initially surrounded by protoplanetary disks. Owing to the preferential formation of stars in stellar clusters, the protoplanetary disks around th…

astro-ph.SR2015★ 76 cited

Strong effect of the cluster environment on the size of protoplanetary discs?

Kirsten Vincke, Andreas Breslau, Susanne Pfalzner

Context. Most stars are born in clusters, thus the protoplanetary discs surrounding the newly formed stars might be influenced by this environment. Isolated star-disc encounters ha…

astro-ph.GA2014★ 82 cited

Sizes of protoplanetary discs after star-disc encounters

Andreas Breslau, Manuel Steinhausen, Kirsten Vincke +1

Most stars do not form in isolation, but as part of a star cluster or association. These young stars are initially surrounded by protoplanetary discs. In these cluster environments…