Astrophysics II

Overview

Advanced stellar structure and evolution: physics of stellar interiors; concepts of single-star evolution; end points of stellar evolution

Radiative transfer: radiative transfer in solar and stellar atmospheres; statistical and ionization equilibrium, plasma diagnostics and line broadening processes

Galaxies: the Milky Way galaxy; galaxy properties; physics of the interstellar medium, theories of galaxy formation and evolution

Learning Objectives

Students will be able to:

Demonstrate a detailed comprehension of the main concepts underpinning modern astrophysics with emphasis on stellar interiors/atmospheres, stellar evolution and galaxy structure / evolution.

Explain the physics of stars and stellar evolution, and be able to describe the physical state of stars at all stages of their lives, and critically compare their fates and the various classes of objects they leave behind.

Understand and be able to link the physical conditions existing in a variety of astrophysics environments, including stellar interiors, stellar atmospheres and galaxies to observations (including spectroscopy) and the principles of radiative transfer.

Describe the properties of galaxies, their constituents and their evolution.

Apply their knowledge to unfamiliar astrophysical problems.

Skills

Problem solving. Searching for and evaluating information from a range of sources. Written communication of scientific concepts in a clear and concise manner. Working independently and meeting deadlines.

Assessment

NONE