Age determination of galaxy merger remnant stars using asteroseismology

The Age and Interior Rotation of Stars from Asteroseismology

Determination of Remnant Merger Stage of Equal-Mass Disk Galaxies

There are many examples of merging galaxy found in observational astronomy, yet the timescales on which merging happens do not allow for one to study the evolution of galaxy merging of any one merger. Furthermore, there are no standard techniques for the identification of the stage of a galaxy mergers progress in the merging process. In this paper, simulations of merging galaxies are analyzed f...

Asteroseismology of Sun-like Stars

In the past decade, helioseismology has revolutionized our understanding of the interior structure of the Sun. In the next decade, asteroseismology will place this knowledge into context, by providing structural information for dozens of pulsating stars across the H-R diagram. Solar-like oscillations have already been detected from the ground in a few stars, and several current and planned sate...

Asteroseismology of close binary stars

In this review paper, we summarise the goals of asteroseismic studies of close binary stars. We first briefly recall the basic principles of asteroseismology, and highlight how the binarity of a star can be an asset, but also a complication, for the interpretation of the stellar oscillations. We discuss a few sample studies of pulsations in close binaries and summarise some case studies. This l...

Asteroseismology of Exoplanets-host Stars

Studying the internal structure of exoplanets-host stars compared to that of similar stars without detected planets is particularly important for the understanding of planetary formation. The observed overmetallicity of stars around which planets have been detected may be a hint in that respect. In this framework, asteroseismic studies represent an excellent tool to determine the structural dif...