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Relating The Origins Of Disk Bar Structure To Star Formation And Stellar Dynamics In Simulations Of Resolved Galaxies

Iles, Elizabeth Jayne Latrobe 北海道大学

2023.03.23

概要

The effects of galactic structure formation and the mechanisms which may
provoke galaxies to evolve into the specific and varied morphologies observable
throughout the universe remains one of the pressing questions in astronomy today. In particular, this work will focus on the presence and effects of the central
bar feature which can be observed in many–although not all–spiral disk-type
galaxies, including the Milky Way. It has been shown that a range of formation
mechanisms can produce such a bar-like feature in the central region of galaxies and consequently, affect the properties of both the host-galaxy and the bar
structure itself (Hohl, 1971; Noguchi, 1987; Raha et al., 1991; Sheth et al., 2002;
Sellwood, 2014; Martinez-Valpuesta et al., 2017; Zana et al., 2019). However,
a comprehensive understanding of how galactic bar formation directly impacts
the interstellar medium (ISM) and correspondingly, star formation and stellar
dynamics in a given galaxy, is still elusive. Additionally, while many previous
studies endeavour to show that the presence of a bar will significantly impact
the general stellar properties in disk galaxies, this is often considered independently of the mechanisms capable of producing such features. This research
aims to investigate whether the different formation mechanisms capable of
producing a central galactic bar also subsequently affect the impact of the bar
on the host-galaxy’s stellar populations and star forming ISM in significant
and discernibly different ways. These features could then become potential
signatures for identifying the origins of any observable barred-system, even
post-interaction, while simultaneously developing the wider understanding of
galactic bars and their ongoing role in galactic evolution.
In recent years, increasingly detailed, high resolution, large-scale observational surveys have continued to raise the ability of astronomers to measure
and assess star formation rates and efficiencies, as well as document the wide
range of observed morphological and dynamical features in galaxies—i.e. ...

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