Katarina Kraljic

Starbursts hiding in the main sequence: a pathway toward quenching?

Star-forming galaxies spend most of their lifetimes on the star-forming main sequence, which establishes a tight empirical and statistical relation between stellar mass and star-formation rate. Occasional episodes of rapid star formation can push them temporarily above this seque...

The evolution of the spin alignments of dark matter halos in the cosmic web

We investigate the evolution of dark matter halo spin alignments with respect to cosmic filaments and explore how halo mass, proximity to filaments, and major mergers affect their orientation over time. We performed a suite of dark matter-only zoom-in N-body simulations centered...

Anisotropy of Satellite Galaxies. I. Contrasting Correlations with Central Galaxy, Host Halo, and Large-scale Filament Structures

Abstract Using the SIMBA, EAGLE, and IllustrisTNG-100 galaxy formation simulations, we examine the anisotropy of the satellite distribution and its dependencies on central galaxies, host halos, and cosmic filaments. We find that in all simulations, the satellite anisotropy is rob...

Zippers and Twisters: Planes of Satellite Galaxies Emerge from Whirling and Shocking Gas Streams in the Cosmic Web

Abstract We investigate dwarf satellite systems around massive centrals analogs (Milky Way to Centaurus A) in the NewHorizon simulation. Using simple estimators limiting overdetection, we identify planes of satellites comparable to observations in 30%–70% of cases. The full sampl...