TL;DR
This paper discusses 3D studies of galaxies in the Local Universe, focusing on neutral hydrogen gas, galaxy morphology, kinematics, and star formation, utilizing new visualization tools and models.
Contribution
Introduces new 3D visualization tools and algorithms for analyzing galaxy morphology and kinematics, aiding current and future large-scale galaxy surveys.
Findings
Enhanced understanding of galaxy structure and gas distribution.
Development of tools for multi-wavelength data visualization.
Insights into galaxy environment effects on star formation.
Abstract
Here I present results from individual galaxy studies and galaxy surveys in the Local Universe with particular emphasis on the spatially resolved properties of neutral hydrogen gas. The 3D nature of the data allows detailed studies of the galaxy morphology and kinematics, their relation to local and global star formation as well as galaxy environments. I use new 3D visualisation tools to present multi-wavelength data, aided by tilted-ring models of the warped galaxy disks. Many of the algorithms and tools currently under development are essential for the exploration of upcoming large survey data, but are also highly beneficial for the analysis of current galaxy surveys.
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