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http://hdl.handle.net/20.500.12386/31794
Title: | Lighting up dark matter haloes | Authors: | DE LUCIA, GABRIELLA | Issue Date: | 2019 | Journal: | GALAXIES | Number: | 7 | Issue: | 2 | Abstract: | Previous chapters of this issue have focused on the formation and evolution of cosmic structures under the influence of gravity alone. In order to make a close link between theoretical models of structure formation and observational data, it is necessary to consider the gas-dynamical and radiative processes that drive the evolution of the baryonic components of dark matter halos. These processes cover many orders of magnitude in physical sizes and time-scales and are entangled in a complex network of actions, back-reactions, and self-regulations. In addition, our understanding of them is far from being complete, even when viewed in isolation. This chapter provides a brief review of the techniques that are commonly used to link the physical properties of galaxies with the dark matter halos in which they reside. I discuss the main features of these methods, as well as their aims, limits, and complementarities. | URI: | http://hdl.handle.net/20.500.12386/31794 | URL: | https://www.mdpi.com/2075-4434/7/2/56/htm https://api.elsevier.com/content/abstract/scopus_id/85069970536 |
ISSN: | 2075-4434 | DOI: | 10.3390/GALAXIES7020056 | Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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galaxies-07-00056.pdf | Pdf editoriale | 3.31 MB | Adobe PDF | View/Open |
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