collaborators

7 papers

astro-ph.GA2026

Expanding stellar associations as Galactic accelerometers

Till Sawala, Núria Miret Roig

The gravitational potential of the Milky Way is fundamental for understanding the evolution of our Galaxy and the nature of dark matter. We introduce a new method to constrain the…

astro-ph.CO2026

The local galaxy distribution does not violate the cosmological principle

Till Sawala

The cosmological principle, which states that the Universe is statistically homogeneous and isotropic on sufficiently large scales, is a foundational assumption of the standard cos…

astro-ph.CO2026

Cylindrical cosmological simulations with StePS

Gábor Rácz, Viola H. Varga, Balázs Pál +3

The global topology of the Universe can affect long-range gravitational forces via boundary conditions. Detailed studies of non-trivial topologies require simulations that natively…

astro-ph.GA2026

Planes of satellites, at once transient and persistent

Till Sawala

The appearance of highly anisotropic planes of satellites around the Milky Way and other galaxies was long considered a challenge to the standard cosmological model. Some recent si…

astro-ph.GA2026

Stellar Cores Live Long and Prosper in Cuspy Dark Matter Halos

Jenni Häkkinen, Alexander Rawlings, Till Sawala +1

The existence of cuspy or cored centers of dark matter halos is a crucial discriminant between different dark matter models. It has recently been claimed based on dynamical argumen…

astro-ph.CO2025

The Giant Arc -- Filament or Figment?

Till Sawala, Meri Teeriaho

The so-called "Giant Arc" is a sparse pattern of MgII absorbers spanning approximately 740 comoving Mpc, whose discovery has been claimed to contradict the large-scale homogeneity…