activity
20162026
most citedNIHAO XIV: Reproducing the observed diversity of dwarf galaxy rotation curve shapes in LCDM

90 citations · 299 across the 22 of their papers we have counts for

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Showing astro-ph.GAShow all

29 papers · 1 filter

astro-ph.GA2026

Forged in Quenching: Morphological Transformation across Star-forming and Quiescent Galaxies in EAGLE

Kai Wang, Carlton Baugh, Sownak Bose +15

The connection between morphology and quenching in central galaxies is well established, but its physical origin remains widely debated. We address this by tracing the main progeni…

astro-ph.GA2026

The descendants of JWST galaxies in the COLIBRE simulations

Xu Zhao, Carlos S. Frenk, Andrew Pontzen +9

Recent observations with JWST have revealed a population of UV-bright galaxies at . This discovery naturally raises the question: what do such early galaxies evolve in…

astro-ph.GA2026

Ruffled Feathers: Merger-driven galaxy size growth and structural transformation in EAGLE

Kai Wang, Carlton Baugh, Sownak Bose +9

Galaxy mergers drive both the size growth and the transformation from discs to spheroids, yet the prescriptions used to model these processes in semi-analytic frameworks have not b…

astro-ph.GA2026

Inflow-driven galaxy evolution - I. Revealing the physics of the fundamental metallicity relation

Kai Wang, Carlton Baugh, N. F. Boardman +11

We present a unified physical framework for the fundamental metallicity relation (FMR), based on the mass-continuity equations. The FMR is not merely the anti-correlation between s…

astro-ph.GA2026

A statistical look on kinematic planes of satellite galaxies II: The physics behind their early formation in TNG50 MW/M31-like galaxies

Matías Gámez-Marín, Rosa Domínguez-Tenreiro, Isabel Santos-Santos +2

We investigate the physical origin of kinematically persistent planes (KPPs) of satellite galaxies in a sample of 190 Milky Way (MW)/M31-like host-satellite systems drawn from the…

astro-ph.GA2026

The missing ultra-faint satellites of the Milky Way

Isabel M. E. Santos-Santos, Carlos S. Frenk, Julio F. Navarro

We combine the highest resolution N-body simulation of a CDM halo (Aquarius-A) with the {\sc GALFORM} galaxy formation semianalytic model to study the f…