most citedRe-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores

25 citations · 33 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2024

Environmental effects on Low Surface Brightness Galaxies in the IllustrisTNG simulation

Luis Enrique Pérez-Montaño, Bernardo Cervantes Sodi, Vicente Rodriguez-Gomez +2

Employing the TNG100 run of the IllustrisTNG project, we characterize the environment of Low Surface Brightness Galaxies (LSBGs) across varying scales, from their associated dark m…

astro-ph.GA2023

Formation of dense filaments induced by runaway supermassive black holes

Go Ogiya, Daisuke Nagai

A narrow linear object extending from the centre of a galaxy at redshift has recently been discovered and interpreted as shocked gas filament formi…

astro-ph.GA20237 cited

Searching for clues of past binary supermassive black hole mergers in nuclear star clusters

Alessandra Mastrobuono-Battisti, Go Ogiya, Oliver Hahn +1

Galaxy mergers are common processes in the Universe. As a large fraction of galaxies hosts at their centres a central supermassive black hole (SMBH), mergers can lead to the format…

astro-ph.GA202216 cited

Shedding light on low-mass subhalo survival and annihilation luminosity with numerical simulations

Alejandra Aguirre-Santaella, Miguel A. Sánchez-Conde, Go Ogiya +2

In this work, we carry out a suite of specially-designed numerical simulations to shed further light on dark matter (DM) subhalo survival at mass scales relevant for gamma-ray DM s…

astro-ph.GA2021

On the Tidal Formation of Dark Matter Deficient Galaxies

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

Previous studies have shown that dark matter deficient galaxies (DMDG) such as NGC1052-DF2 (hereafter DF2) can result from tidal stripping. An important question, though, is whethe…

astro-ph.GA201425 cited

Re-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores

Go Ogiya, Andreas Burkert

Recent studies found the densities of dark matter (DM) subhaloes which surround nearby dwarf spheroidal galaxies (dSphs) to be significantly lower than those of the most massive su…