The host galaxies of Compact Steep Spectrum and Gigahertz-Peaked Spectrum radio sources
J. Holt
TL;DR
This review discusses the properties of host galaxies of CSS and GPS radio sources, emphasizing their morphology, stellar content, and gas properties to understand galaxy evolution and the role of young radio-loud AGN.
Contribution
It provides a comprehensive overview of host galaxy characteristics of CSS and GPS sources, focusing on their implications for galaxy evolution.
Findings
Host galaxies of CSS and GPS sources show diverse morphologies.
These galaxies contain significant stellar and gas components.
Young radio-loud AGN are crucial for understanding galaxy evolution.
Abstract
I will review some of the developments in studies of the host galaxy properties of Compact Steep Spectrum (CSS) and GigaHertz-Peaked Spectrum (GPS) radio sources. In contrast to previous reviews structured around observational technique, I will discuss the host galaxy properties in terms of morphology, stellar content and warm gas properties and discuss how compact, young radio-loud AGN are key objects for understanding galaxy evolution.
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