Module Specifications.
Current Academic Year 2024 - 2025
All Module information is indicative, and this portal is an interim interface pending the full upgrade of Coursebuilder and subsequent integration to the new DCU Student Information System (DCU Key).
As such, this is a point in time view of data which will be refreshed periodically. Some fields/data may not yet be available pending the completion of the full Coursebuilder upgrade and integration project. We will post status updates as they become available. Thank you for your patience and understanding.
Date posted: September 2024
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Repeat examination |
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Description This module focuses on a general understanding of the properties of galaxies and the intergalactic medium, along with the different observational techniques used to study them. | |||||||||||||||||||||||||||||||||||||||||||
Learning Outcomes 1. Interpret basic astronomical data, extract relevant parameters 2. Assess the most appropriate observational techniques for variety of systems. 3. Explain galactic rotation and discuss the impact of dark-matter on rotation curves. 4. Describe the different building blocks of galaxies 5. Summarise the formation processes of galaxies, and their impact on observables. 6. Understand the role of magnetic fields in different cosmic environments 7. Discuss the nature of the intergalactic medium on different cosmic scales and times | |||||||||||||||||||||||||||||||||||||||||||
All module information is indicative and subject to change. For further information,students are advised to refer to the University's Marks and Standards and Programme Specific Regulations at: http://www.dcu.ie/registry/examinations/index.shtml |
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Indicative Content and Learning Activities
GalaxiesStructure of galaxies, galactic rotation curves, dark matter, formation of galaxies, active galactic nucleiObservational techniquesTelescopes, photometry, spectroscopy, interferometry, signal-to-noise, data reduction, comparing data to modelsThe intergalactic mediumThe intracluster medium, filaments of the large scale structure, the “missing baryon” problem.Cosmic magnetic fieldsMagnetic fields in galaxies and the intergalactic medium, origin and evolution of magnetic fields. | |||||||||||||||||||||||||||||||||||||||||||
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Indicative Reading List
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Other Resources None | |||||||||||||||||||||||||||||||||||||||||||