PHY213 - Stellar Structure and Evolution

Nebula - NASA/ESA and the Hubble Heritage Team (AURA/STScI)/HEIC

Module Summary

This course aims to provide an understanding of the physical processes occurring in stars which are responsible for their internal structure, plus the evolutionary path followed by a low mass star from the main sequence to a white dwarf and the evolution of massive stars leading to neutron star or black hole remnants.


Module Description


Timetable information for this module can be found listed here

Course material

Course material is hosted on MOLE