AS5522 Stellar Physics
Academic year
2025 to 2026 Semester 2
Curricular information may be subject to change
Further information on which modules are specific to your programme.
Key module information
SCOTCAT credits
15
SCQF level
SCQF level 11
Availability restrictions
Available only to students on MSc Astrophysics.
Module description
This module develops the physics of stellar interiors and atmospheres from the basic equations of stellar structure and radiative transfer concepts developed in Nebulae and Stars I. Topics include: the equation of state that provides pressure support at the high temperatures and densities found in normal and white-dwarf stars; the interaction of radiation with matter, both in terms of radiation-pressure support in super-massive stars and in terms of the role of opacity in controlling the flow of energy from the stellar interior to the surface; the equation of radiative transfer and the effects of local temperatures, pressures and velocity fields on the continuum and line absorption profiles in the emergent spectrum. Computer-aided tutorial exercises illustrate the computational schemes that represent one of the triumphs of late twentieth-century physics, in their ability to predict the observable properties of a star from its radius and luminosity, which in turn are determined by its mass, age and chemical composition.
Relationship to other modules
Pre-requisites
STUDENTS MUST BE REGISTERED FOR MSC ASTROPHYSICS.
Co-requisites
YOU MUST ALSO TAKE AS5500
Assessment pattern
2-hour Written Examination = 75%, Coursework = 25%
Re-assessment
Oral re-assessment = 100%, capped at grade 7
Learning and teaching methods and delivery
Weekly contact
3 lectures occasionally replaced by whole-group tutorials.
Scheduled learning hours
33
Guided independent study hours
117