Abstract
The detailed dynamical structure of the bulge in the Milky Way is currently under debate. Although kinematics of the bulge stars can be well reproduced by a boxy-bulge, the possible existence of a small embedded classical bulge can not be ruled out. We study the dynamical evolution of a small classical bulge in a model of the Milky Way using a self-consistent high resolution N-body simulation. Detailed kinematics and dynamical properties of such a bulge are presented. © Owned by the authors, published by EDP Sciences, 2012.
Cite
CITATION STYLE
Saha, K., Martinez-Valpuesta, I., & Gerhard, O. (2012). Dynamical evolution of a bulge in an N-body model of the Milky Way. In EPJ Web of Conferences (Vol. 19). https://doi.org/10.1051/epjconf/20121906008
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.