activity
20042025
most citedA Revised Model for the Formation of Disk Galaxies: Low Spin and Dark-Halo Expansion

280 citations · 847 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2025★ 1 cited

Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50

Isabel Medlock, Daisuke Nagai, Nir Mandelker +4

Cold, dense streams of gas are predicted to penetrate deeply into massive halos (> 10^12 Msun) at cosmic noon (z=4-2), fueling galaxies to sustain high star formation rates. We inv…

astro-ph.GA2025★ 5 cited

Dynamics in the Cores of Self-Interacting Dark Matter Halos: Reduced Stalling and Accelerated Core Collapse

Frank C. van den Bosch, Shashank Dattathri

Self-interacting dark matter (SIDM) is an intriguing alternative to the standard cold dark matter (CDM) paradigm, which predicts that dark matter halos typically have large, isothe…

astro-ph.GA2025

The Impact of Baryonic Effects on the Dynamical Masses Inferred Using Satellite Kinematics

Josephine F. W. Baggen, Frank C. van den Bosch, Kaustav Mitra

Satellite kinematics offers a powerful method to infer dynamical halo masses and has been demonstrated to yield tight constraints on the galaxy-halo connection. However, previous s…

astro-ph.GA2025★ 1 cited

The Dipole Instability in Gravitational -body Systems: A Natural Explanation for Lopsidedness and Off-Centered Nuclei in Galaxies

Shashank Dattathri, Frank C. van den Bosch, Martin D. Weinberg +1

We explore the stability of isotropic, spherical, self-gravitating systems with a double-power law density profile. Systems with rapid transitions between the inner and outer slope…

astro-ph.GA2024★ 1 cited

The tidal evolution of anisotropic subhaloes: A new pathway to creating isotropic and cored satellites

Barry T. Chiang, Frank C. van den Bosch, Hsi-Yu Schive

It is common practice, both in dynamical modelling and in idealised numerical simulations, to assume that galaxies and/or dark matter haloes are spherical and have isotropic veloci…

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…