activity
19962023
most citedAn expanded M_bh-sigma diagram, and a new calibration of active galactic nuclei masses

424 citations · 1.5k across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.GA2023

Roman Early-Definition Astrophysics Survey Opportunity: Galactic Roman Infrared Plane Survey (GRIPS)

Roberta Paladini, Catherine Zucker, Robert Benjamin +67

A wide-field near-infrared survey of the Galactic disk and bulge/bar(s) is supported by a large representation of the community of Galactic astronomers. The combination of sensitiv…

astro-ph.GA2020★ 8 cited

Basis function expansions for galactic dynamics: Spherical versus cylindrical coordinates

Yougang Wang, E. Athanassoula, Shude Mao

Aims. The orbital structure of galaxies is strongly influenced by the accuracy of the force calculation during orbit integration. We explore the accuracy of force calculations for…

astro-ph.GA2017★ 16 cited

Forming disc galaxies in major mergers: III. The effect of angular momentum on the radial density profiles of disc galaxies

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

We study the effect of angular momentum on the surface density profiles of disc galaxies, using high resolution simulations of major mergers whose remnants have downbending radial…

astro-ph.GA2016★ 22 cited

Orbital classification in an N-body bar

Yougang Wang, E. Athanassoula, Shude Mao

The dynamics and evolution of any galactic structure are strongly influenced by the properties of the orbits that constitute it. In this paper, we compare two orbit classification…

astro-ph.GA2015★ 33 cited

Applying Schwarzschild's orbit superposition method to barred or non-barred disc galaxies

Eugene Vasiliev, E. Athanassoula

We present an implementation of the Schwarzschild orbit superposition method which can be used for constructing self-consistent equilibrium models of barred or non-barred disc gala…

astro-ph.GA2014★ 97 cited

Adventures of a tidally induced bar

E. L. Lokas, E. Athanassoula, V. P. Debattista +5

Using N-body simulations, we study the properties of a bar induced in a dwarf galaxy as a result of tidal interaction with the Milky Way. The dwarf is initially composed of a disk…