activity
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

collaborators
Showing 2015 · astro-ph.GAShow all

12 papers · 2 filters

astro-ph.GA2015★ 73 cited

APOGEE Kinematics I: Overview of the Kinematics of the Galactic Bulge as Mapped by APOGEE

M. Ness, G. Zasowski, J. A. Johnson +12

We present the stellar kinematics across the Galactic bulge and into the disk at positive longitudes from the SDSS-III APOGEE spectroscopic survey of the Milky Way. APOGEE includes…

astro-ph.GA2015★ 8 cited

Globular Cluster Populations: Results Including SG Late-Type Galaxies

Dennis Zaritsky, Kelsey McCabe, Manuel Aravena +18

Using 3.6 and 4.5m images of 73 late-type, edge-on galaxies from the SG survey, we compare the richness of the globular cluster populations of these galaxies to those of ear…

astro-ph.GA2015

Spectral analysis of stellar orbits in a tidally induced bar

Grzegorz Gajda, Ewa L. Lokas, E. Athanassoula

Using numerical analysis of fundamental frequencies we study the orbital structure of a tidally induced bar formed in a simulated dwarf galaxy orbiting a Milky Way-like host. We fi…

astro-ph.GA2015★ 87 cited

Environmental regulation of cloud and star formation in galactic bars

F. Renaud, F. Bournaud, E. Emsellem +7

The strong time-dependence of the dynamics of galactic bars yields a complex and rapidly evolving distribution of dense gas and star forming regions. Although bars mainly host regi…

astro-ph.GA2015★ 8 cited

The Odd Offset between the Galactic Disk and Its Bar in NGC 3906

Bonita de Swardt, Kartik Sheth, Taehyun Kim +27

We use mid-infrared 3.6 and 4.5microns imaging of NGC 3906 from the Spitzer Survey of Stellar Structure in Galaxies (S4G) to understand the nature of an unusual offset between its…

astro-ph.GA2015★ 2 cited

The Spitzer Survey of Stellar Structure in Galaxies (S4G): Stellar Masses, Sizes and Radial Profiles for 2352 Nearby Galaxies

Juan Carlos Munoz-Mateos, Kartik Sheth, Michael Regan +25

The Spitzer Survey of Stellar Structure in Galaxies (S4G) is a volume, magnitude, and size-limited survey of 2352 nearby galaxies with deep imaging at 3.6 and 4.5um. In this paper…

astro-ph.GA2015

Stellar Populations of Barred Quiescent Galaxies

Edmond Cheung, Charlie Conroy, E. Athanassoula +10

Selecting centrally quiescent galaxies from the Sloan Digital Sky Survey (SDSS) to create high signal-to-noise (>100) stacked spectra with minimal emission line contamination, we a…

astro-ph.GA2015★ 46 cited

H-alpha kinematics of S4G spiral galaxies-II. Data description and non-circular motions

Santiago Erroz-Ferrer, Johan H. Knapen, Ryan Leaman +15

We present a kinematical study of 29 spiral galaxies included in the Spitzer Survey of Stellar Structure in Galaxies, using Halpha Fabry-Perot data obtained with the Galaxy Halpha…

astro-ph.GA2015★ 72 cited

2D kinematic signatures of boxy/peanut bulges

Francesca Iannuzzi, E. Athanassoula

We study the imprints of boxy/peanut structures on the 2D line-of-sight kinematics of simulated disk galaxies. The models under study belong to a family with varying initial gas fr…

astro-ph.GA2015★ 45 cited

Boxy/peanut/X bulges, barlenses and the thick part of galactic bars: What are they and how did they form?

E. Athanassoula

Bars have a complex three-dimensional shape. In particular their inner part is vertically much thicker than the parts further out. Viewed edge-on, the thick part of the bar is what…

astro-ph.GA2015★ 38 cited

The Effects of Boxy/Peanut Bulges on Galaxy Models

F. Fragkoudi, E. Athanassoula, A. Bosma +1

We examine the effects that the modelling of a Boxy/Peanut (B/P) bulge will have on the estimates of the stellar gravitational potential, forces, orbital structure and bar strength…

astro-ph.GA2015★ 336 cited

A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)

R. Buta, K. Sheth, E. Athanassoula +22

The Spitzer Survey of Stellar Structure in Galaxies (S4G) is the largest available database of deep, homogeneous middle-infrared (mid-IR) images of galaxies of all types. The surve…