activity
19952026
most citedThe Structure of Dark Matter Haloes in Dwarf Galaxies

1.4k citations · 22.5k across the 252 of their papers we have counts for

collaborators

252 papers

astro-ph.GA2026

The Merger-Driven Origin of the Vast Extended Stellar Disc Around the Andromeda Galaxy

C. Tsakonas, M. Arnaboldi, F. Hammer +4

The closest giant spiral, the Andromeda galaxy (M31), shows compelling evidence for a recent, gas-rich major merger event. Pronounced substructures in its inner halo and a kinemati…

astro-ph.GA2023★ 6 cited

Mapping gravity in stellar nurseries -- establishing the effectiveness of 2D acceleration maps

Zhen-Zhen He, Guang-Xing Li, Andreas Burkert

Gravity is the driving force of star formation. Although gravity is caused by the presence of matter, its role in complex regions is still unsettled. One effective way to study the…

astro-ph.GA2023★ 6 cited

Filament fragmentation: Density gradients suppress end dominated collapse

Elena Hoemann, Stefan Heigl, Andreas Burkert

The onset of star formation is set by the collapse of filaments in the interstellar medium. From a theoretical point of view, an isolated cylindrical filament forms cores via the e…

astro-ph.GA2023★ 2 cited

The Orbital Structure and Selection Effects of the Galactic Center S-Star Cluster

Andreas Burkert, Stefan Gillessen, Douglas N. C. Lin +4

The orbital distribution of the S-star cluster surrounding the supermassive black hole in the center of the Milky Way is analyzed. A tight, roughly exponential dependence of the pe…

astro-ph.GA2022★ 10 cited

Testing the galaxy collision induced formation scenario for the trail of dark matter deficient galaxies with the susceptibility of globular clusters to the tidal force

Go Ogiya, Frank C. van den Bosch, Andreas Burkert +1

It has been suggested that a trail of diffuse galaxies, including two dark matter deficient galaxies (DMDGs), in the vicinity of NGC1052 formed because of a high-speed collision be…

astro-ph.GA2022★ 8 cited

Characterizing the 3D Kinematics of Young Stars in the Radcliffe Wave

Alan J. Tu, Catherine Zucker, Joshua S. Speagle +5

We present an analysis of the kinematics of the Radcliffe Wave, a 2.7-kpc-long sinusoidal band of molecular clouds in the solar neighborhood recently detected via 3D dust mapping.…