activity
20172025
most citedGalaxies with prolate rotation in Illustris

34 citations · 84 across the 4 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA202033 cited

Revealing the Structure and Internal Rotation of the Sagittarius Dwarf Spheroidal Galaxy with Gaia and Machine Learning

Andrés del Pino, Mark A. Fardal, Roeland P. van der Marel +3

We present a detailed study of the internal structure and kinematics of the core of the Sagittarius dwarf spheroidal galaxy (Sgr). Using machine-learning techniques, we have combin…

astro-ph.GA2019

Dark matter distribution and dynamics of dwarf spheroidal galaxies

Ewa L. Lokas

I review the current status of dynamical modelling of dwarf spheroidal galaxies focusing on estimates of their dark matter content. Starting with the simplest methods using the vel…

astro-ph.GA2019

Anatomy of a buckling galactic bar

Ewa L. Lokas

Using -body simulations we study the buckling instability in a galactic bar forming in a Milky Way-like galaxy. The galaxy is initially composed of an axisymmetric, exponential…

astro-ph.GA201917 cited

Buckling instability in tidally induced galactic bars

Ewa L. Lokas

Strong galactic bars produced in simulations tend to undergo a period of buckling instability that weakens and thickens them and forms a boxy/peanut structure in their central part…

astro-ph.GA2018

The major merger origin of the Andromeda II kinematics

Ivana Ebrová, Ewa L. Łokas, Sylvain Fouquet +1

Prolate rotation (i.e. rotation around the long axis) has been reported for two Local Group dwarf galaxies: Andromeda II, a dwarf spheroidal satellite of M31, and Phoenix, a transi…

astro-ph.GA2018

Tidally induced bars in gas-rich dwarf galaxies orbiting the Milky Way

Grzegorz Gajda, Ewa L. Łokas, E. Athanassoula

Bars in galaxies may form not only through instability, but also as a result of an interaction with another galaxy. In particular, they may appear in disky dwarf galaxies interacti…