University of St Andrews

Key information

SCOTCAT credits : 15

ECTS credits : 7

Level : SCQF level 11

Semester: 2

Planned timetable: To be arranged.

This theoretical module explores the basics of gravitational dynamics and accretion physics and their application to systems such as circumstellar discs, stellar clusters to galaxies and clusters of galaxies. The module will provide students with the techniques to determine physical properties from observable quantities and to model the dynamics and evolutionary pathways of these systems. Starting from two-body motion and orbits under a central-force law, the module describes the calculation of extended potentials and their associated orbits. The use of the virial theorem and the statistical treatment of large numbers of self-gravitating bodies is then developed with application to stellar systems. Accretion as a source of energy and mass growth will be explored with particular emphasis on models of viscous accretion discs. Applications of these methods are made to several different astrophysical objects including accretion discs in stellar systems , collisions in globular clusters, the growth of super-massive black holes, to the presence of dark matter in the universe.

Relationship to other modules

Co-requisite(s): You must also take AS5500

Learning and teaching methods and delivery

Weekly contact: 3-hour lectures (x 11 weeks), 1-hour tutorials (x 5 weeks)

Scheduled learning hours: 38

Guided independent study hours: 112

Assessment pattern

As used by St Andrews: 2-hour Written Examination = 75%, Coursework = 25%

As defined by QAA
Written examinations : 75%
Practical examinations : 0%
Coursework: 25%

Personnel

Module coordinator: Professor I A Bonnell
Module teaching staff: Prof I Bonnell