The Structure of Galaxies

Code School Level Credits Semesters
PHYS3011 Physics and Astronomy 3 10 Spring UK
Code
PHYS3011
School
Physics and Astronomy
Level
3
Credits
10
Semesters
Spring UK

Summary

This module develops the current understanding of the various physical processes that dictate the formation, evolution and structure of galaxies. The layout of the course is as follows: The Milky Way (structure, components, HI kinematics); Basic Properties of Galaxies (morphology, classification schemes, constituents); The Dynamics of Galaxies (gaseous and stellar kinematics, galaxy rotation curves, spiral structure and bar formation, the virial theorem); Active Galaxies (Seyfert galaxies, unified model, radio galaxies, BL Lac objects, quasars, supermassive black holes); The Environment of Galaxies (The Local Group, galaxy clustering and large-scale structure, X-ray properties of clusters, galaxy mergers, the morphology-density relation); Galaxy Evolution (monolithic and hierarchical models, evidence for evolution from nearby galaxies, observations of distant galaxies).

 

 

 

 

 

Target Students

Students on Part I and Part II of single honours Physics courses.

Classes

This module is based on a series of lectures throughout the spring semester.

Assessment

Assessed by end of spring semester

Educational Aims

To introduce the ideas behind current theories of the formation, evolution and structure of galaxies.

Learning Outcomes

Knowledge and Understanding: 

On successful completion of the module, students will have enhanced their: 

Intellectual Skills:  

On successful completion of the module, students will have demonstrated their ability to: 

Professional/Practical Skills:

On successful completion of the module, students will have demonstrated their ability to: 

Transferable/Key Skills:  

On successful completion of the module, students will have demonstrated their ability to: 

Conveners

View in Curriculum Catalogue
Last updated 07/01/2025.