activity
20142021
most citedDynamical modelling of the Galactic bulge and bar: the Milky Way's bar pattern speed, stellar, and dark matter mass distribution

380 citations · 816 across the 8 of their papers we have counts for

collaborators

7 papers

astro-ph.GA201614 cited

Peanut-shaped metallicity distributions in bulges of edge-on galaxies: the case of NGC 4710

Oscar A. Gonzalez, Victor P. Debattista, Melissa Ness +2

Bulges of edge-on galaxies are often boxy/peanut-shaped (B/PS), and unsharp masks reveal the presence of an X shape. Simulations show that these shapes can be produced by dynamical…

astro-ph.IM2016214 cited

The GALAH Survey: Observational Overview and Gaia DR1 companion

Sarah Martell, Sanjib Sharma, Sven Buder +30

The Galactic Archaeology with HERMES (GALAH) Survey is a massive observational project to trace the Milky Way's history of star formation, chemical enrichment, stellar migration an…

astro-ph.GA201698 cited

A radial age gradient in the geometrically thick disk of the Milky Way

Marie Martig, Ivan Minchev, Melissa Ness +2

In the Milky Way, the thick disk can be defined using individual stellar abundances, kinematics, or age; or geometrically, as stars high above the mid-plane. In nearby galaxies, wh…

astro-ph.GA2016380 cited

Dynamical modelling of the Galactic bulge and bar: the Milky Way's bar pattern speed, stellar, and dark matter mass distribution

Matthieu Portail, Ortwin Gerhard, Christopher Wegg +1

We construct a large set of dynamical models of the galactic bulge, bar and inner disk using the Made-to-Measure method. Our models are constrained to match the red clump giant den…

astro-ph.GA201446 cited

The X-Shaped Milky Way Bulge in OGLE-III Photometry and in N-Body Models

David M. Nataf, Andrzej Udalski, Jan Skowron +11

We model the split red clump of the Galactic bulge in OGLE-III photometry, and compare the results to predictions from two N-body models. Our analysis yields precise maps of the br…

astro-ph.GA201437 cited

Dissecting galactic bulges in space and time I: the importance of early formation scenarios vs. secular evolution

M. K. Seidel, R. Cacho, T. Ruiz-Lara +7

The details of bulge formation via collapse, mergers, secular processes or their interplay remain unresolved. To start answering this question and quantify the importance of distin…