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19962026
most citedWhat determines the strength and the slowdown rate of bars ?

597 citations · 11.5k across the 182 of their papers we have counts for

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Showing 2018 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2018★ 85 cited

SDSS-IV MaNGA: pattern speeds of barred galaxies

Rui Guo, Shude Mao, E. Athanassoula +5

The MaNGA project has obtained IFU data for several thousand nearby galaxies, including barred galaxies. With the two dimensional spectral and kinematic information provided by IFU…

astro-ph.GA2018★ 68 cited

Linking bar- and interaction-driven molecular gas concentration with centrally-enhanced star formation in EDGE-CALIFA galaxies

Ryan Chown, Cheng Li, E. Athanassoula +6

We study the spatially resolved star formation history and molecular gas distribution of 58 nearby galaxies, using integral field spectroscopy from the CALIFA survey and CO $J=1\ri…

astro-ph.GA2018★ 10 cited

Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations

P. Ramirez-Moreta, L. Verdes-Montenegro, J. Blasco-Herrera +21

Asymmetries in HI in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project h…

astro-ph.GA2018★ 18 cited

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…

astro-ph.GA2018★ 19 cited

Tidally induced morphology of M33 in hydrodynamical simulations of its recent interaction with M31

Marcin Semczuk, Ewa L. Lokas, Jean-Baptiste Salomon +2

We present a hydrodynamical model of M33 and its recent interaction with M31. This scenario was previously proposed in the literature in order to explain the distorted gaseous and…

astro-ph.GA2018★ 1 cited

Using N-body simulations to understand the chemo-dynamical evolution of the inner Milky Way

E. Athanassoula

I present examples of how chemo-dynamical N-body simulations can help understanding the structure and evolution of the inner Galaxy. Such simulations reproduce the observed links b…