Module overview
We will start from outlining fundamental questions we must answer in order to build up a picture of an astrophysical object, e.g., what is it made of? How luminous? How big? How old? How fast? How heavy? These seemingly simple questions are surprisingly difficult to answer but we will cover the different astrophysical tools used to answer them.
We will then move outwards to consider the demography, spatial distribution, and environment of galaxies, in the ‘field’ and in clusters. We will then consider galaxies very distant from us in space and time, discuss galaxy formation and evolution, and have an overview of Active Galaxies, super-massive black holes and their co-evolution with their host galaxies.
Linked modules
Pre-requisite: PHYS1005
Aims and Objectives
Learning Outcomes
Subject Specific Intellectual and Research Skills
Having successfully completed this module you will be able to:
- Outline the relationships between dark matter, galaxies, and the large-scale structure of the Universe
- Investigate the physics behind galaxy motions
- Interpret the structural and evolutionary differences of spiral and elliptical galaxies
- Differentiate the relevant physical processes in active galaxies
Transferable and Generic Skills
Having successfully completed this module you will be able to:
- Develop mathematical tools for applied physics
- Formulate links between statistics and physics
Knowledge and Understanding
Having successfully completed this module, you will be able to demonstrate knowledge and understanding of:
- Main families of high-redshift galaxies
- The structural, morphological, environmental, and spectral differences of galaxies.
- The differences between the spectra of stars and galaxies.
- Environment of galaxies and its connection to galaxy evolution
Syllabus
- The make-up of galaxies: stars, gas, dust and dark matter.
- Galaxy morphology: Luminosities and sizes, surface brightness, elliptical galaxies, spirals, irregular galaxies, galaxy masses.
- Basic galaxy dynamics: The virial theorem
- Galaxy demographics: Demographics of different types of galaxies, luminosity functions, surveys.
- Galaxy environment: large-scale structure, clustering, clusters and groups, effect on galaxies.
- Galaxy groups and clusters : Scaling relations, mass estimates.
- The cosmological setting of galaxies: Distance measurements, cosmological redshift, Hubble expansion of the universe.
- Active galaxies and supermassive black holes : Supermassive black holes in normal and active galaxies, quasars, radio galaxies, unification, the possible role of AGN in galaxy evolution.
- Galaxy evolution: Hierarchical structure formation and Galaxy mergers and interactions, galaxies at high-redhisft, cosmic downsizing, star formation history of the universe.
Learning and Teaching
Teaching and learning methods
Q&As via zappers
In-class group activities
On-line group activities
Blogs
Videos, Movies
| Type | Hours |
|---|---|
| Revision | 10 |
| Preparation for scheduled sessions | 18 |
| Completion of assessment task | 16 |
| Lecture | 36 |
| Wider reading or practice | 52 |
| Follow-up work | 18 |
| Total study time | 150 |
Resources & Reading list
General Resources
Web-sites of additional Lectures. Provided in class..
Module notes on Blackboards.
Textbooks
Galaxies & Galactic Structure. Elmegreen.
Galaxy Formation and Evolution. Mo, van den Bosch, White.
The Structure and Evolution of galaxies. Phillips.
S S Sparke & J S Gallagher (2007). Galaxies in the universe: an introduction. Cambridge University Press.
An introduction to modern astrophysics. Carroll & Ostlie.
Assessment
Summative
This is how we’ll formally assess what you have learned in this module.
| Method | Percentage contribution |
|---|---|
| Continuous Assessment | 20% |
| Final Assessment | 80% |
Referral
This is how we’ll assess you if you don’t meet the criteria to pass this module.
| Method | Percentage contribution |
|---|---|
| Set Task | 100% |
Repeat
An internal repeat is where you take all of your modules again, including any you passed. An external repeat is where you only re-take the modules you failed.
| Method | Percentage contribution |
|---|---|
| Set Task | 100% |
Repeat Information
Repeat type: Internal & External