Observable Properties of Double-Barred Galaxies in N-Body Simulations

TL;DR

This study uses N-body simulations to analyze the properties and dynamics of double-barred galaxies, providing insights into their structure, kinematics, and rotation patterns, and comparing results with observations.

Contribution

It characterizes the density and kinematic properties of simulated double-barred galaxies, enhancing understanding and comparison with observed systems.

Findings

Simulated secondary bars have sizes and shapes consistent with observations.

Weak kinematic twists suggest decoupled secondary bars produce subtle velocity field signatures.

Non-rigid rotation affects pattern speed measurements, with some bars possibly rotating oppositely.

Abstract

Although at least one quarter of early-type barred galaxies host secondary stellar bars embedded in their large-scale primary counterparts, the dynamics of such double barred galaxies are still not well understood. Recently we reported success at simulating such systems in a repeatable way in collisionless systems. In order to further our understanding of double-barred galaxies, here we characterize the density and kinematics of the N-body simulations of these galaxies. This will facilitate comparison with observations and lead to a better understanding of the observed double-barred galaxies. We find the shape and size of our simulated secondary bars are quite reasonable compared to the observed ones. We demonstrate that an authentic decoupled secondary bar may produce only a weak twist of the kinematic minor axis in the stellar velocity field, due to the relatively large random motion of stars in the central region. We also find that the edge-on nuclear bars are probably not related to boxy peanut-shaped bulges which are most likely to be edge-on primary large-scale bars. Finally we demonstrate that the non-rigid rotation of the secondary bar causes its pattern speed not to be derived with great accuracy using the Tremaine-Weinberg method. We also compare with observations of NGC 2950, a prototypical double-barred early-type galaxy, which suggest that the nuclear bar may be rotating in the opposite sense as the primary.