Résumé / Abstract Journal-club_Galaxies

Séminaire/Seminar Galaxies

« Connecting the Progenitors of Cosmic Web across Cosmic Time »

Hannah Jhee
Department of Physics, University of Seoul (Séoul, Corée du Sud)

Galaxy halos evolve differently according to the environment
they live in, while the environment itself evolves as well. While it is
known that large-scale filaments are, as highly anisotropic environments,
responsible for changing in halos' orbital motion, morphology, spin or
mass, structural evolution effect is underestimated so far. In this work,
using DisPerSE, we extract filament structures from smoothed density fields
from z=0 to z=3. Each filament structure at each snapshot, starting from a
node and ending at another node, is reconstructed using critical point
information, and their progenitors are traced based on similarities in
spatial extent. From the constructed trees of filament, we examine
individual detailed properties of the densities, radii and velocities, and
how these evolution affects nearby halos.
jeudi 1 février 2024 - 11:30
Salle des séminaires Évry Schatzman
Institut d'Astrophysique de Paris
Page web du séminaire / Seminar's webpage