activity
20172022
most citedDisruption of Dark Matter Substructure: Fact or Fiction?

317 citations · 760 across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.GA202210 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.GA202117 cited

Evolution of subhalo orbits in a smoothly-growing host halo potential

Go Ogiya, James E. Taylor, Michael J. Hudson

The orbital parameters of dark matter (DM) subhaloes play an essential role in determining their mass-loss rates and overall spatial distribution within a host halo. Haloes in cosm…

astro-ph.GA2020

Dynamical self-friction: how mass loss slows you down

Tim B. Miller, Frank C. van den Bosch, Sheridan B. Green +1

We investigate dynamical self-friction, the process by which material that is stripped from a subhalo torques its remaining bound remnant, which causes it to lose orbital angular m…

astro-ph.GA201932 cited

Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters

Go Ogiya, Oliver Hahn, Chiara M. F. Mingarelli +1

The coalescence of supermassive black holes (SMBHs) should generate the strongest sources of gravitational waves (GWs) in the Universe. However, the dynamics of their coalescence i…

astro-ph.GA201953 cited

DASH: a library of dynamical subhalo evolution

Go Ogiya, Frank C. van den Bosch, Oliver Hahn +3

The abundance and demographics of dark matter substructure is important for many areas in astrophysics and cosmological -body simulations have been the primary tool used to inve…

astro-ph.GA2018

Tidal stripping as a possible origin of the ultra diffuse galaxy lacking dark matter

Go Ogiya

Recent observations revealed a mysterious ultra diffuse galaxy, NGC1052-DF2, in the group of a large elliptical galaxy, NGC1052. Compared to expectations from abundance matching mo…