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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 2017Show all

5 papers · 1 filter

astro-ph.GA2017★ 9 cited

An Overview of the MHONGOOSE Survey: Observing Nearby Galaxies with MeerKAT

W. J. G. de Blok, E. A. K. Adams, P. Amram +65

MHONGOOSE is a deep survey of the neutral hydrogen distribution in a representative sample of 30 nearby disk and dwarf galaxies with HI masses from 10^6 to ~10^{11} M_sun, and lumi…

astro-ph.GA2017★ 44 cited

Morphology and enhanced star formation in a Cartwheel-like ring galaxy

F. Renaud, E. Athanassoula, P. Amram +8

We use hydrodynamical simulations of a Cartwheel-like ring galaxy, modelled as a nearly head-on collision of a small companion with a larger disc galaxy, to probe the evolution of…

astro-ph.GA2017★ 32 cited

How do spiral arm contrasts relate to bars, disk breaks and other fundamental galaxy properties?

Adrian Bittner, Dimitri A. Gadotti, Bruce G. Elmegreen +4

We investigate how the properties of spiral arms relate to other fundamental galaxy properties, including bars and disc breaks. We use previously published measurements of those pr…

astro-ph.GA2017★ 31 cited

Tidally induced bars in dwarf galaxies on different orbits around a Milky Way-like host

Grzegorz Gajda, Ewa L. Lokas, E. Athanassoula

Bars in galaxies may develop through a global instability or due to an interaction with another system. We study bar formation in disky dwarf galaxies orbiting a Milky Way-like gal…

astro-ph.GA2017★ 7 cited

Forming disc galaxies in major mergers II. The central mass concentration problem and a comparison of GADGET3 with GIZMO

S. A. Rodionov, E. Athanassoula, N. Peschken

Context: In a series of papers, we study the major merger of two disk galaxies in order to establish whether or not such a merger can produce a disc galaxy. Aims: Our aim here is t…